Contains a record describing each AtlasOutline objec
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| objID | long | Unique Id number, composed of rerun, run, camcol, field, objid | ||||
| size | int | number of spans allocated | ||||
| nspan | int | actual number of spans | ||||
| row0 | int | row offset from parent region | ||||
| col0 | int | col offset from parent region | ||||
| rmin | int | pix | bounding box min row | |||
| rmax | int | pix | bounding box max row | |||
| cmin | int | pix | bounding box min col | |||
| cmax | int | pix | bounding box max col | |||
| npix | int | pix | number of pixels in object | |||
| span | string | span data as string |
Every column of every table has a description in this tabl
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| tablename | string | The name of the parent table | ||||
| name | string | The name of column | ||||
| unit | string | Optional description of units | ||||
| ucd | string | Optional UCD definition | ||||
| enum | string | Optional link to an enumerated table | ||||
| description | string | One line description of column | ||||
| rank | int | Optional position of column in table column display |
Every SkyServer database object has a one line description in this tabl
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| name | string | Name of the object | ||||
| type | string | Its system type | ||||
| access | string | Defines user or admin access | ||||
| description | string | One line description of contents | ||||
| text | string | Detailed description of contents | ||||
| rank | int | Optional position of column in table display |
The columns of each view are stored for the auto-documentatio
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| name | string | The name of column | ||||
| viewname | string | The name of the view | ||||
| parent | string | The name of the parent |
The table stores the values of various enumerated and bitmask columnns
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| field | string | Field Name | ||||
| name | string | Constant Name | ||||
| value | int | Type value | ||||
| description | string | Short description |
Contains the detailed inventory of database object
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| filename | string | The name of the sql file | ||||
| parent | string | Name of caller | ||||
| child | string | Name of called function |
This table stores a full diagnostic snapshot of the database
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| name | string | Name of object | ||||
| type | string | System type of the object (U:table, V:view, F: function, P: stored proc) | ||||
| count | long | Optional row count, where applicable |
SDSS objects that match to FIRST objects have their match parameters stored her
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| objID | long | unique id, points to photoObj | ||||
| ra | double | deg | FIRST source right ascension, J2000 | |||
| dec | double | deg | FIRST source declination, J2000 | |||
| warning | string | warning in FIRST catalog | ||||
| peak | float | mJy | Peak FIRST radio flux | |||
| integr | float | mJy | Integrated FIRST radio flux | |||
| rms | float | mJy | rms error in flux | |||
| major | float | arcsec | Major axis (deconvolved) | |||
| minor | float | arcsec | Minor axis (deconvolved) | |||
| pa | float | deg | position angle (east of north) | |||
| skyrms | float | mJy | background rms error in flux |
All the measured parameters and calibrations of a photometric fiel
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| fieldID | long | Unique SDSS identifier composed from [skyVersion,rerun,run,camcol,field]. | ||||
| skyVersion | int | Layer of catalog (currently only one layer, 0; 0-15 available) | ||||
| run | int | Run number | ||||
| rerun | int | Rerun number | ||||
| camcol | int | Camera column | ||||
| field | int | Field number | ||||
| nTotal | int | Number of total objects in the field | ||||
| nObjects | int | Number of non-bright objects in the field | ||||
| nChild | int | Number of "child" objects in the field | ||||
| nGalaxy | int | Number of objects classified as "galaxy" | ||||
| nStars | int | Number of objects classified as "star" | ||||
| nCR_u | int | Number of cosmics in u-band | ||||
| nCR_g | int | Number of cosmics in g-band | ||||
| nCR_r | int | Number of cosmics in r-band | ||||
| nCR_i | int | Number of cosmics in i-band | ||||
| nCR_z | int | Number of cosmics in z-band | ||||
| nBrightObj_u | int | Number of bright objects in u-band | ||||
| nBrightObj_g | int | Number of bright objects in g-band | ||||
| nBrightObj_r | int | Number of bright objects in r-band | ||||
| nBrightObj_i | int | Number of bright objects in i-band | ||||
| nBrightObj_z | int | Number of bright objects in z-band | ||||
| nFaintObj_u | int | Number of faint objects in u-band | ||||
| nFaintObj_g | int | Number of faint objects in g-band | ||||
| nFaintObj_r | int | Number of faint objects in r-band | ||||
| nFaintObj_i | int | Number of faint objects in i-band | ||||
| nFaintObj_z | int | Number of faint objects in z-band | ||||
| quality | int | Quality of field | ||||
| mjd_u | double | MJD(TAI) when row 0 of u-band field was read | ||||
| mjd_g | double | MJD(TAI) when row 0 of g-band field was read | ||||
| mjd_r | double | MJD(TAI) when row 0 of r-band field was read | ||||
| mjd_i | double | MJD(TAI) when row 0 of i-band field was read | ||||
| mjd_z | double | MJD(TAI) when row 0 of z-band field was read | ||||
| a_u | float | a term in astrometry for u-band | ||||
| a_g | float | a term in astrometry for g-band | ||||
| a_r | float | a term in astrometry for r-band | ||||
| a_i | float | a term in astrometry for i-band | ||||
| a_z | float | a term in astrometry for z-band | ||||
| b_u | float | b term in astrometry for u-band | ||||
| b_g | float | b term in astrometry for g-band | ||||
| b_r | float | b term in astrometry for r-band | ||||
| b_i | float | b term in astrometry for i-band | ||||
| b_z | float | b term in astrometry for z-band | ||||
| c_u | float | c term in astrometry for u-band | ||||
| c_g | float | c term in astrometry for g-band | ||||
| c_r | float | c term in astrometry for r-band | ||||
| c_i | float | c term in astrometry for i-band | ||||
| c_z | float | c term in astrometry for z-band | ||||
| d_u | float | d term in astrometry for u-band | ||||
| d_g | float | d term in astrometry for g-band | ||||
| d_r | float | d term in astrometry for r-band | ||||
| d_i | float | d term in astrometry for i-band | ||||
| d_z | float | d term in astrometry for z-band | ||||
| e_u | float | e term in astrometry for u-band | ||||
| e_g | float | e term in astrometry for g-band | ||||
| e_r | float | e term in astrometry for r-band | ||||
| e_i | float | e term in astrometry for i-band | ||||
| e_z | float | e term in astrometry for z-band | ||||
| f_u | float | f term in astrometry for u-band | ||||
| f_g | float | f term in astrometry for g-band | ||||
| f_r | float | f term in astrometry for r-band | ||||
| f_i | float | f term in astrometry for i-band | ||||
| f_z | float | f term in astrometry for z-band | ||||
| dRow0_u | float | Zero-order row distortion coefficient in u-band | ||||
| dRow0_g | float | Zero-order row distortion coefficient in g-band | ||||
| dRow0_r | float | Zero-order row distortion coefficient in r-band | ||||
| dRow0_i | float | Zero-order row distortion coefficient in i-band | ||||
| dRow0_z | float | Zero-order row distortion coefficient in z-band | ||||
| dRow1_u | float | First-order row distortion coefficient in u-band | ||||
| dRow1_g | float | First-order row distortion coefficient in g-band | ||||
| dRow1_r | float | First-order row distortion coefficient in r-band | ||||
| dRow1_i | float | First-order row distortion coefficient in i-band | ||||
| dRow1_z | float | First-order row distortion coefficient in z-band | ||||
| dRow2_u | float | Second-order row distortion coefficient in u-band | ||||
| dRow2_g | float | Second-order row distortion coefficient in g-band | ||||
| dRow2_r | float | Second-order row distortion coefficient in r-band | ||||
| dRow2_i | float | Second-order row distortion coefficient in i-band | ||||
| dRow2_z | float | Second-order row distortion coefficient in z-band | ||||
| dRow3_u | float | Third-order row distortion coefficient in u-band | ||||
| dRow3_g | float | Third-order row distortion coefficient in g-band | ||||
| dRow3_r | float | Third-order row distortion coefficient in r-band | ||||
| dRow3_i | float | Third-order row distortion coefficient in i-band | ||||
| dRow3_z | float | Third-order row distortion coefficient in z-band | ||||
| dCol0_u | float | Zero-order column distortion coefficient in u-band | ||||
| dCol0_g | float | Zero-order column distortion coefficient in g-band | ||||
| dCol0_r | float | Zero-order column distortion coefficient in r-band | ||||
| dCol0_i | float | Zero-order column distortion coefficient in i-band | ||||
| dCol0_z | float | Zero-order column distortion coefficient in z-band | ||||
| dCol1_u | float | First-order column distortion coefficient in u-band | ||||
| dCol1_g | float | First-order column distortion coefficient in g-band | ||||
| dCol1_r | float | First-order column distortion coefficient in r-band | ||||
| dCol1_i | float | First-order column distortion coefficient in i-band | ||||
| dCol1_z | float | First-order column distortion coefficient in z-band | ||||
| dCol2_u | float | Second-order column distortion coefficient in u-band | ||||
| dCol2_g | float | Second-order column distortion coefficient in g-band | ||||
| dCol2_r | float | Second-order column distortion coefficient in r-band | ||||
| dCol2_i | float | Second-order column distortion coefficient in i-band | ||||
| dCol2_z | float | Second-order column distortion coefficient in z-band | ||||
| dCol3_u | float | Third-order column distortion coefficient in u-band | ||||
| dCol3_g | float | Third-order column distortion coefficient in g-band | ||||
| dCol3_r | float | Third-order column distortion coefficient in r-band | ||||
| dCol3_i | float | Third-order column distortion coefficient in i-band | ||||
| dCol3_z | float | Third-order column distortion coefficient in z-band | ||||
| csRow_u | float | Slope in row DCR correction for blue objects (u-band) | ||||
| csRow_g | float | Slope in row DCR correction for blue objects (g-band) | ||||
| csRow_r | float | Slope in row DCR correction for blue objects (r-band) | ||||
| csRow_i | float | Slope in row DCR correction for blue objects (i-band) | ||||
| csRow_z | float | Slope in row DCR correction for blue objects (z-band) | ||||
| csCol_u | float | Slope in column DCR correction for blue objects (u-band) | ||||
| csCol_g | float | Slope in column DCR correction for blue objects (g-band) | ||||
| csCol_r | float | Slope in column DCR correction for blue objects (r-band) | ||||
| csCol_i | float | Slope in column DCR correction for blue objects (i-band) | ||||
| csCol_z | float | Slope in column DCR correction for blue objects (z-band) | ||||
| ccRow_u | float | Constant row DCR correction for blue objects (u-band) | ||||
| ccRow_g | float | Constant row DCR correction for blue objects (g-band) | ||||
| ccRow_r | float | Constant row DCR correction for blue objects (r-band) | ||||
| ccRow_i | float | Constant row DCR correction for blue objects (i-band) | ||||
| ccRow_z | float | Constant row DCR correction for blue objects (z-band) | ||||
| ccCol_u | float | Constant column DCR correction for blue objects (u-band) | ||||
| ccCol_g | float | Constant column DCR correction for blue objects (g-band) | ||||
| ccCol_r | float | Constant column DCR correction for blue objects (r-band) | ||||
| ccCol_i | float | Constant column DCR correction for blue objects (i-band) | ||||
| ccCol_z | float | Constant column DCR correction for blue objects (z-band) | ||||
| riCut_u | float | r-i cutoff between blue and red objects (for u-band astrometry) | ||||
| riCut_g | float | r-i cutoff between blue and red objects (for g-band astrometry) | ||||
| riCut_r | float | r-i cutoff between blue and red objects (for r-band astrometry) | ||||
| riCut_i | float | r-i cutoff between blue and red objects (for i-band astrometry) | ||||
| riCut_z | float | r-i cutoff between blue and red objects (for z-band astrometry) | ||||
| airmass_u | float | mag | Airmass for star at frame center (midway through u-band exposure) | |||
| airmass_g | float | mag | Airmass for star at frame center (midway through g-band exposure) | |||
| airmass_r | float | mag | Airmass for star at frame center (midway through r-band exposure) | |||
| airmass_i | float | mag | Airmass for star at frame center (midway through i-band exposure) | |||
| airmass_z | float | mag | Airmass for star at frame center (midway through z-band exposure) | |||
| muErr_u | float | arcsec | Error in mu in astrometric calibration (for u-band) | |||
| muErr_g | float | arcsec | Error in mu in astrometric calibration (for g-band) | |||
| muErr_r | float | arcsec | Error in mu in astrometric calibration (for r-band) | |||
| muErr_i | float | arcsec | Error in mu in astrometric calibration (for i-band) | |||
| muErr_z | float | arcsec | Error in mu in astrometric calibration (for z-band) | |||
| nuErr_u | float | arcsec | Error in nu in astrometric calibration (for u-band) | |||
| nuErr_g | float | arcsec | Error in nu in astrometric calibration (for g-band) | |||
| nuErr_r | float | arcsec | Error in nu in astrometric calibration (for r-band) | |||
| nuErr_i | float | arcsec | Error in nu in astrometric calibration (for i-band) | |||
| nuErr_z | float | arcsec | Error in nu in astrometric calibration (for z-band) | |||
| ra | double | deg | Center RA of field | |||
| dec | double | deg | Center Dec of field | |||
| raMin | double | deg | Minimum RA of field | |||
| raMax | double | deg | Maximum RA of field | |||
| decMin | double | deg | Minimum Dec of field | |||
| decMax | double | deg | Maximum Dec of field | |||
| pixScale | double | arcsec/pix | Mean size of pixel (r-band) | |||
| primaryArea | double | deg^2 | Area covered by primary part of field | |||
| photoStatus | int | Frames processing status bitmask | ||||
| rowOffset_u | float | pix | Offset to add to transformed row coordinates (u-band) | |||
| rowOffset_g | float | pix | Offset to add to transformed row coordinates (g-band) | |||
| rowOffset_r | float | pix | Offset to add to transformed row coordinates (r-band) | |||
| rowOffset_i | float | pix | Offset to add to transformed row coordinates (i-band) | |||
| rowOffset_z | float | pix | Offset to add to transformed row coordinates (z-band) | |||
| colOffset_u | float | pix | Offset to add to transformed row coordinates (u-band) | |||
| colOffset_g | float | pix | Offset to add to transformed row coordinates (g-band) | |||
| colOffset_r | float | pix | Offset to add to transformed row coordinates (r-band) | |||
| colOffset_i | float | pix | Offset to add to transformed row coordinates (i-band) | |||
| colOffset_z | float | pix | Offset to add to transformed row coordinates (z-band) | |||
| saturationLevel_u | int | counts | Saturation level in u-band | |||
| saturationLevel_g | int | counts | Saturation level in g-band | |||
| saturationLevel_r | int | counts | Saturation level in r-band | |||
| saturationLevel_i | int | counts | Saturation level in i-band | |||
| saturationLevel_z | int | counts | Saturation level in z-band | |||
| nEffPsf_u | float | pix | Effective area of PSF (u-band) | |||
| nEffPsf_g | float | pix | Effective area of PSF (g-band) | |||
| nEffPsf_r | float | pix | Effective area of PSF (r-band) | |||
| nEffPsf_i | float | pix | Effective area of PSF (i-band) | |||
| nEffPsf_z | float | pix | Effective area of PSF (z-band) | |||
| skyPsp_u | float | nmgy/arcsec^2 | Sky estimate from PSP (u-band) | |||
| skyPsp_g | float | nmgy/arcsec^2 | Sky estimate from PSP (g-band) | |||
| skyPsp_r | float | nmgy/arcsec^2 | Sky estimate from PSP (r-band) | |||
| skyPsp_i | float | nmgy/arcsec^2 | Sky estimate from PSP (i-band) | |||
| skyPsp_z | float | nmgy/arcsec^2 | Sky estimate from PSP (z-band) | |||
| skyFrames_u | float | nmgy/arcsec^2 | Frames sky value | |||
| skyFrames_g | float | nmgy/arcsec^2 | Frames sky value | |||
| skyFrames_r | float | nmgy/arcsec^2 | Frames sky value | |||
| skyFrames_i | float | nmgy/arcsec^2 | Frames sky value | |||
| skyFrames_z | float | nmgy/arcsec^2 | Frames sky value | |||
| skyFramesSub_u | float | nmgy/arcsec^2 | Frames sky value after object subtraction | |||
| skyFramesSub_g | float | nmgy/arcsec^2 | Frames sky value after object subtraction | |||
| skyFramesSub_r | float | nmgy/arcsec^2 | Frames sky value after object subtraction | |||
| skyFramesSub_i | float | nmgy/arcsec^2 | Frames sky value after object subtraction | |||
| skyFramesSub_z | float | nmgy/arcsec^2 | Frames sky value after object subtraction | |||
| sigPix_u | float | nmgy/arcsec^2 | Sigma of pixel values in u-band frame (clipped) | |||
| sigPix_g | float | nmgy/arcsec^2 | Sigma of pixel values in g-band frame (clipped) | |||
| sigPix_r | float | nmgy/arcsec^2 | Sigma of pixel values in r-band frame (clipped) | |||
| sigPix_i | float | nmgy/arcsec^2 | Sigma of pixel values in i-band frame (clipped) | |||
| sigPix_z | float | nmgy/arcsec^2 | Sigma of pixel values in z-band frame (clipped) | |||
| devApCorrection_u | float | deV aperture correction (u-band) | ||||
| devApCorrection_g | float | deV aperture correction (g-band) | ||||
| devApCorrection_r | float | deV aperture correction (r-band) | ||||
| devApCorrection_i | float | deV aperture correction (i-band) | ||||
| devApCorrection_z | float | deV aperture correction (z-band) | ||||
| devApCorrectionErr_u | float | Error in deV aperture correction (u-band) | ||||
| devApCorrectionErr_g | float | Error in deV aperture correction (g-band) | ||||
| devApCorrectionErr_r | float | Error in deV aperture correction (r-band) | ||||
| devApCorrectionErr_i | float | Error in deV aperture correction (i-band) | ||||
| devApCorrectionErr_z | float | Error in deV aperture correction (z-band) | ||||
| expApCorrection_u | float | exponential aperture correction (u-band) | ||||
| expApCorrection_g | float | exponential aperture correction (g-band) | ||||
| expApCorrection_r | float | exponential aperture correction (r-band) | ||||
| expApCorrection_i | float | exponential aperture correction (i-band) | ||||
| expApCorrection_z | float | exponential aperture correction (z-band) | ||||
| expApCorrectionErr_u | float | Error in exponential aperture correction (u-band) | ||||
| expApCorrectionErr_g | float | Error in exponential aperture correction (g-band) | ||||
| expApCorrectionErr_r | float | Error in exponential aperture correction (r-band) | ||||
| expApCorrectionErr_i | float | Error in exponential aperture correction (i-band) | ||||
| expApCorrectionErr_z | float | Error in exponential aperture correction (z-band) | ||||
| devModelApCorrection_u | float | model aperture correction, for deV case (u-band) | ||||
| devModelApCorrection_g | float | model aperture correction, for deV case (g-band) | ||||
| devModelApCorrection_r | float | model aperture correction, for deV case (r-band) | ||||
| devModelApCorrection_i | float | model aperture correction, for deV case (i-band) | ||||
| devModelApCorrection_z | float | model aperture correction, for deV case (z-band) | ||||
| devModelApCorrectionErr_u | float | Error in model aperture correction, for deV case (u-band) | ||||
| devModelApCorrectionErr_g | float | Error in model aperture correction, for deV case (g-band) | ||||
| devModelApCorrectionErr_r | float | Error in model aperture correction, for deV case (r-band) | ||||
| devModelApCorrectionErr_i | float | Error in model aperture correction, for deV case (i-band) | ||||
| devModelApCorrectionErr_z | float | Error in model aperture correction, for deV case (z-band) | ||||
| expModelApCorrection_u | float | model aperture correction, for exponential case (u-band) | ||||
| expModelApCorrection_g | float | model aperture correction, for exponential case (g-band) | ||||
| expModelApCorrection_r | float | model aperture correction, for exponential case (r-band) | ||||
| expModelApCorrection_i | float | model aperture correction, for exponential case (i-band) | ||||
| expModelApCorrection_z | float | model aperture correction, for exponential case (z-band) | ||||
| expModelApCorrectionErr_u | float | Error in model aperture correction, for exponential case (u-band) | ||||
| expModelApCorrectionErr_g | float | Error in model aperture correction, for exponential case (g-band) | ||||
| expModelApCorrectionErr_r | float | Error in model aperture correction, for exponential case (r-band) | ||||
| expModelApCorrectionErr_i | float | Error in model aperture correction, for exponential case (i-band) | ||||
| expModelApCorrectionErr_z | float | Error in model aperture correction, for exponential case (z-band) | ||||
| medianFiberColor_u | float | Median fiber magnitude of objects (u-band) | ||||
| medianFiberColor_g | float | Median fiber magnitude of objects (g-band) | ||||
| medianFiberColor_r | float | Median fiber magnitude of objects (r-band) | ||||
| medianFiberColor_i | float | Median fiber magnitude of objects (i-band) | ||||
| medianFiberColor_z | float | Median fiber magnitude of objects (z-band) | ||||
| medianPsfColor_u | float | Median PSF magnitude of objects (u-band) | ||||
| medianPsfColor_g | float | Median PSF magnitude of objects (g-band) | ||||
| medianPsfColor_r | float | Median PSF magnitude of objects (r-band) | ||||
| medianPsfColor_i | float | Median PSF magnitude of objects (i-band) | ||||
| medianPsfColor_z | float | Median PSF magnitude of objects (z-band) | ||||
| q_u | float | Means Stokes Q parameter in u-band frame | ||||
| q_g | float | Means Stokes Q parameter in g-band frame | ||||
| q_r | float | Means Stokes Q parameter in r-band frame | ||||
| q_i | float | Means Stokes Q parameter in i-band frame | ||||
| q_z | float | Means Stokes Q parameter in z-band frame | ||||
| u_u | float | Means Stokes U parameter in u-band frame | ||||
| u_g | float | Means Stokes U parameter in g-band frame | ||||
| u_r | float | Means Stokes U parameter in r-band frame | ||||
| u_i | float | Means Stokes U parameter in i-band frame | ||||
| u_z | float | Means Stokes U parameter in z-band frame | ||||
| pspStatus | int | Maximum value of PSP (Postage Stamp Pipeline) status over all 5 filters | ||||
| sky_u | float | nmgy/arcsec^2 | PSP estimate of sky in u-band | |||
| sky_g | float | nmgy/arcsec^2 | PSP estimate of sky in g-band | |||
| sky_r | float | nmgy/arcsec^2 | PSP estimate of sky in r-band | |||
| sky_i | float | nmgy/arcsec^2 | PSP estimate of sky in i-band | |||
| sky_z | float | nmgy/arcsec^2 | PSP estimate of sky in z-band | |||
| skySig_u | float | mag | Fractional Sigma of Sky Value Distribution, expressed as magnitude. Sky noise = skySig * sky * ln(10)/2.5 | |||
| skySig_g | float | mag | Fractional Sigma of Sky Value Distribution, expressed as magnitude. Sky noise = skySig * sky * ln(10)/2.5 | |||
| skySig_r | float | mag | Fractional Sigma of Sky Value Distribution, expressed as magnitude. Sky noise = skySig * sky * ln(10)/2.5 | |||
| skySig_i | float | mag | Fractional Sigma of Sky Value Distribution, expressed as magnitude. Sky noise = skySig * sky * ln(10)/2.5 | |||
| skySig_z | float | mag | Fractional Sigma of Sky Value Distribution, expressed as magnitude. Sky noise = skySig * sky * ln(10)/2.5 | |||
| skyErr_u | float | nmgy/arcsec^2 | Error in PSP estimate of sky in u-band | |||
| skyErr_g | float | nmgy/arcsec^2 | Error in PSP estimate of sky in g-band | |||
| skyErr_r | float | nmgy/arcsec^2 | Error in PSP estimate of sky in r-band | |||
| skyErr_i | float | nmgy/arcsec^2 | Error in PSP estimate of sky in i-band | |||
| skyErr_z | float | nmgy/arcsec^2 | Error in PSP estimate of sky in z-band | |||
| skySlope_u | float | nmgy/arcsec^2/field | Rate of change in sky value along columns (u-band) | |||
| skySlope_g | float | nmgy/arcsec^2/field | Rate of change in sky value along columns (g-band) | |||
| skySlope_r | float | nmgy/arcsec^2/field | Rate of change in sky value along columns (r-band) | |||
| skySlope_i | float | nmgy/arcsec^2/field | Rate of change in sky value along columns (i-band) | |||
| skySlope_z | float | nmgy/arcsec^2/field | Rate of change in sky value along columns (z-band) | |||
| lbias_u | float | ADUs | Left-hand amplifier bias level (u-band) XXX make sure to apply DSCALE, counts or ADU? | |||
| lbias_g | float | ADUs | Left-hand amplifier bias level (g-band) | |||
| lbias_r | float | ADUs | Left-hand amplifier bias level (r-band) | |||
| lbias_i | float | ADUs | Left-hand amplifier bias level (i-band) | |||
| lbias_z | float | ADUs | Left-hand amplifier bias level (z-band) | |||
| rbias_u | float | ADUs | Right-hand amplifier bias level (u-band) | |||
| rbias_g | float | ADUs | Right-hand amplifier bias level (g-band) | |||
| rbias_r | float | ADUs | Right-hand amplifier bias level (r-band) | |||
| rbias_i | float | ADUs | Right-hand amplifier bias level (i-band) | |||
| rbias_z | float | ADUs | Right-hand amplifier bias level (z-band) | |||
| nProf_u | int | Number of bins in PSF profile (in fieldProfile table) | ||||
| nProf_g | int | Number of bins in PSF profile (in fieldProfile table) | ||||
| nProf_r | int | Number of bins in PSF profile (in fieldProfile table) | ||||
| nProf_i | int | Number of bins in PSF profile (in fieldProfile table) | ||||
| nProf_z | int | Number of bins in PSF profile (in fieldProfile table) | ||||
| psfNStar_u | int | Number of stars used in PSF measurement (u-band) | ||||
| psfNStar_g | int | Number of stars used in PSF measurement (g-band) | ||||
| psfNStar_r | int | Number of stars used in PSF measurement (r-band) | ||||
| psfNStar_i | int | Number of stars used in PSF measurement (i-band) | ||||
| psfNStar_z | int | Number of stars used in PSF measurement (z-band) | ||||
| psfApCorrectionErr_u | float | mag | Photometric uncertainty due to imperfect PSF model (u-band) | |||
| psfApCorrectionErr_g | float | mag | Photometric uncertainty due to imperfect PSF model (g-band) | |||
| psfApCorrectionErr_r | float | mag | Photometric uncertainty due to imperfect PSF model (r-band) | |||
| psfApCorrectionErr_i | float | mag | Photometric uncertainty due to imperfect PSF model (i-band) | |||
| psfApCorrectionErr_z | float | mag | Photometric uncertainty due to imperfect PSF model (z-band) | |||
| psfSigma1_u | float | arcsec | Inner gaussian sigma for composite fit | |||
| psfSigma1_g | float | arcsec | Inner gaussian sigma for composite fit | |||
| psfSigma1_r | float | arcsec | Inner gaussian sigma for composite fit | |||
| psfSigma1_i | float | arcsec | Inner gaussian sigma for composite fit | |||
| psfSigma1_z | float | arcsec | Inner gaussian sigma for composite fit | |||
| psfSigma2_u | float | arcsec | Outer gaussian sigma for composite fit | |||
| psfSigma2_g | float | arcsec | Outer gaussian sigma for composite fit | |||
| psfSigma2_r | float | arcsec | Outer gaussian sigma for composite fit | |||
| psfSigma2_i | float | arcsec | Outer gaussian sigma for composite fit | |||
| psfSigma2_z | float | arcsec | Outer gaussian sigma for composite fit | |||
| psfB_u | float | Ratio of inner to outer components at origin (composite fit) | ||||
| psfB_g | float | Ratio of inner to outer components at origin (composite fit) | ||||
| psfB_r | float | Ratio of inner to outer components at origin (composite fit) | ||||
| psfB_i | float | Ratio of inner to outer components at origin (composite fit) | ||||
| psfB_z | float | Ratio of inner to outer components at origin (composite fit) | ||||
| psfP0_u | float | Value of power law at origin in composite fit XXX | ||||
| psfP0_g | float | Value of power law at origin in composite fit XXX | ||||
| psfP0_r | float | Value of power law at origin in composite fit XXX | ||||
| psfP0_i | float | Value of power law at origin in composite fit XXX | ||||
| psfP0_z | float | Value of power law at origin in composite fit XXX | ||||
| psfBeta_u | float | Slope of power law in composite fit | ||||
| psfBeta_g | float | Slope of power law in composite fit | ||||
| psfBeta_r | float | Slope of power law in composite fit | ||||
| psfBeta_i | float | Slope of power law in composite fit | ||||
| psfBeta_z | float | Slope of power law in composite fit | ||||
| psfSigmaP_u | float | Width of power law in composite fit | ||||
| psfSigmaP_g | float | Width of power law in composite fit | ||||
| psfSigmaP_r | float | Width of power law in composite fit | ||||
| psfSigmaP_i | float | Width of power law in composite fit | ||||
| psfSigmaP_z | float | Width of power law in composite fit | ||||
| psfWidth_u | float | arcsec | Effective PSF width from 2-Gaussian fit (u-band) | |||
| psfWidth_g | float | arcsec | Effective PSF width from 2-Gaussian fit (g-band) | |||
| psfWidth_r | float | arcsec | Effective PSF width from 2-Gaussian fit (r-band) | |||
| psfWidth_i | float | arcsec | Effective PSF width from 2-Gaussian fit (i-band) | |||
| psfWidth_z | float | arcsec | Effective PSF width from 2-Gaussian fit (z-band) | |||
| psfPsfCounts_u | float | counts | Flux via fit to PSF (u-band) XXX | |||
| psfPsfCounts_g | float | counts | Flux via fit to PSF (g-band) XXX | |||
| psfPsfCounts_r | float | counts | Flux via fit to PSF (r-band) XXX | |||
| psfPsfCounts_i | float | counts | Flux via fit to PSF (i-band) XXX | |||
| psfPsfCounts_z | float | counts | Flux via fit to PSF (z-band) XXX | |||
| psf2GSigma1_u | float | arcsec | Sigma of inner gaussian in 2-Gaussian fit (u-band) | |||
| psf2GSigma1_g | float | arcsec | Sigma of inner gaussian in 2-Gaussian fit (g-band) | |||
| psf2GSigma1_r | float | arcsec | Sigma of inner gaussian in 2-Gaussian fit (r-band) | |||
| psf2GSigma1_i | float | arcsec | Sigma of inner gaussian in 2-Gaussian fit (i-band) | |||
| psf2GSigma1_z | float | arcsec | Sigma of inner gaussian in 2-Gaussian fit (z-band) | |||
| psf2GSigma2_u | float | arcsec | Sigma of outer gaussian in 2-Gaussian fit (u-band) | |||
| psf2GSigma2_g | float | arcsec | Sigma of outer gaussian in 2-Gaussian fit (g-band) | |||
| psf2GSigma2_r | float | arcsec | Sigma of outer gaussian in 2-Gaussian fit (r-band) | |||
| psf2GSigma2_i | float | arcsec | Sigma of outer gaussian in 2-Gaussian fit (i-band) | |||
| psf2GSigma2_z | float | arcsec | Sigma of outer gaussian in 2-Gaussian fit (z-band) | |||
| psf2GB_u | float | Ratio of inner to outer components at origin (2-Gaussian fit) | ||||
| psf2GB_g | float | Ratio of inner to outer components at origin (2-Gaussian fit) | ||||
| psf2GB_r | float | Ratio of inner to outer components at origin (2-Gaussian fit) | ||||
| psf2GB_i | float | Ratio of inner to outer components at origin (2-Gaussian fit) | ||||
| psf2GB_z | float | Ratio of inner to outer components at origin (2-Gaussian fit) | ||||
| psfCounts_u | float | counts | PSF counts XXX | |||
| psfCounts_g | float | counts | PSF counts XXX | |||
| psfCounts_r | float | counts | PSF counts XXX | |||
| psfCounts_i | float | counts | PSF counts XXX | |||
| psfCounts_z | float | counts | PSF counts XXX | |||
| gain_u | float | electrons/DN | Gain averaged over amplifiers | |||
| gain_g | float | electrons/DN | Gain averaged over amplifiers | |||
| gain_r | float | electrons/DN | Gain averaged over amplifiers | |||
| gain_i | float | electrons/DN | Gain averaged over amplifiers | |||
| gain_z | float | electrons/DN | Gain averaged over amplifiers | |||
| darkVariance_u | float | Dark variance | ||||
| darkVariance_g | float | Dark variance | ||||
| darkVariance_r | float | Dark variance | ||||
| darkVariance_i | float | Dark variance | ||||
| darkVariance_z | float | Dark variance | ||||
| score | float | Quality of field (0-1) | ||||
| aterm_u | float | nmgy/count | nanomaggies per count due to instrument | |||
| aterm_g | float | nmgy/count | nanomaggies per count due to instrument | |||
| aterm_r | float | nmgy/count | nanomaggies per count due to instrument | |||
| aterm_i | float | nmgy/count | nanomaggies per count due to instrument | |||
| aterm_z | float | nmgy/count | nanomaggies per count due to instrument | |||
| kterm_u | float | atmospheric k-term at reference time in calibration | ||||
| kterm_g | float | atmospheric k-term at reference time in calibration | ||||
| kterm_r | float | atmospheric k-term at reference time in calibration | ||||
| kterm_i | float | atmospheric k-term at reference time in calibration | ||||
| kterm_z | float | atmospheric k-term at reference time in calibration | ||||
| kdot_u | float | 1/second | linear time variation of atmospheric k-term | |||
| kdot_g | float | 1/second | linear time variation of atmospheric k-term | |||
| kdot_r | float | 1/second | linear time variation of atmospheric k-term | |||
| kdot_i | float | 1/second | linear time variation of atmospheric k-term | |||
| kdot_z | float | 1/second | linear time variation of atmospheric k-term | |||
| reftai_u | double | second | reference TAI used for k-term | |||
| reftai_g | double | second | reference TAI used for k-term | |||
| reftai_r | double | second | reference TAI used for k-term | |||
| reftai_i | double | second | reference TAI used for k-term | |||
| reftai_z | double | second | reference TAI used for k-term | |||
| tai_u | double | second | TAI used for k-term | |||
| tai_g | double | second | TAI used for k-term | |||
| tai_r | double | second | TAI used for k-term | |||
| tai_i | double | second | TAI used for k-term | |||
| tai_z | double | second | TAI used for k-term | |||
| nStarsOffset_u | int | number of stars used for fieldOffset determination | ||||
| nStarsOffset_g | int | number of stars used for fieldOffset determination | ||||
| nStarsOffset_r | int | number of stars used for fieldOffset determination | ||||
| nStarsOffset_i | int | number of stars used for fieldOffset determination | ||||
| nStarsOffset_z | int | number of stars used for fieldOffset determination | ||||
| fieldOffset_u | float | mag | offset of field from initial calibration (final minus initial magnitudes) | |||
| fieldOffset_g | float | mag | offset of field from initial calibration (final minus initial magnitudes) | |||
| fieldOffset_r | float | mag | offset of field from initial calibration (final minus initial magnitudes) | |||
| fieldOffset_i | float | mag | offset of field from initial calibration (final minus initial magnitudes) | |||
| fieldOffset_z | float | mag | offset of field from initial calibration (final minus initial magnitudes) | |||
| calibStatus_u | int | calibration status bitmask | ||||
| calibStatus_g | int | calibration status bitmask | ||||
| calibStatus_r | int | calibration status bitmask | ||||
| calibStatus_i | int | calibration status bitmask | ||||
| calibStatus_z | int | calibration status bitmask | ||||
| imageStatus_u | int | image status bitmask | ||||
| imageStatus_g | int | image status bitmask | ||||
| imageStatus_r | int | image status bitmask | ||||
| imageStatus_i | int | image status bitmask | ||||
| imageStatus_z | int | image status bitmask | ||||
| nMgyPerCount_u | float | nmgy/count | nanomaggies per count in u-band | |||
| nMgyPerCount_g | float | nmgy/count | nanomaggies per count in g-band | |||
| nMgyPerCount_r | float | nmgy/count | nanomaggies per count in r-band | |||
| nMgyPerCount_i | float | nmgy/count | nanomaggies per count in i-band | |||
| nMgyPerCount_z | float | nmgy/count | nanomaggies per count in z-band | |||
| nMgyPerCountIvar_u | float | (nmgy/count)^{-2} | Inverse variance of nanomaggies per count in u-band | |||
| nMgyPerCountIvar_g | float | (nmgy/count)^{-2} | Inverse variance of nanomaggies per count in g-band | |||
| nMgyPerCountIvar_r | float | (nmgy/count)^{-2} | Inverse variance of nanomaggies per count in r-band | |||
| nMgyPerCountIvar_i | float | (nmgy/count)^{-2} | Inverse variance of nanomaggies per count in i-band | |||
| nMgyPerCountIvar_z | float | (nmgy/count)^{-2} | Inverse variance of nanomaggies per count in z-band | |||
| ifield | int | field id used by resolve pipeline | ||||
| muStart | double | arcsec | start of field in stripe coords (parallel to scan direction, 64 pixels clipped) | |||
| muEnd | double | arcsec | end of field in stripe coords (parallel to scan direction, 64 pixels clipped) | |||
| nuStart | double | arcsec | start of field in stripe coords (perpendicular to scan direction, 64 pixels clipped) | |||
| nuEnd | double | arcsec | end of field in stripe coords (perpendicular to scan direction, 64 pixels clipped) | |||
| ifindx | int | first entry for this field in the "findx" table matching fields and balkans | ||||
| nBalkans | int | number of balkans contained in this field (and corresponding number of entries in the "findx" table) | ||||
| loadVersion | int | Load Version |
The mean PSF profile for the field as determined from bright stars
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| bin | int | bin number (0..14) | ||||
| band | int | u,g,r,i,z (0..4) | ||||
| profMean | float | nmgy/arcsec^2 | Mean pixel flux in annulus | |||
| profMed | float | nmgy/arcsec^2 | Median profile | |||
| profSig | float | nmgy/arcsec^2 | Sigma of profile | |||
| fieldID | long | links to the field object |
For 'big' databases, maps big tables to their own file group
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| tableName | string | name of table or index | ||||
| tableFileGroup | string | name of filegroup | ||||
| indexFileGroup | string | name of the index filegroup | ||||
| comment | string | explanation |
Contains JPEG images of fields at various zoom factors, and their astrometry
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| fieldID | long | Link to the field table | ||||
| zoom | int | Zoom level 2^(zoom/10) | ||||
| run | int | Run number | ||||
| rerun | int | Rerun number | ||||
| camcol | int | Camera column | ||||
| field | int | Field number | ||||
| stripe | int | Stripe number | ||||
| strip | string | Strip number (N or S) | ||||
| a | double | deg | Astrometric coefficient | |||
| b | double | deg/pix | Astrometric coefficient | |||
| c | double | deg/pix | Astrometric coefficient | |||
| d | double | deg | Astrometric coefficient | |||
| e | double | deg/pix | Astrometric coefficient | |||
| f | double | deg/pix | Astrometric coefficient | |||
| node | double | deg | Astrometric coefficient | |||
| incl | double | deg | Astrometric coefficient | |||
| raMin | double | deg | Min of ra | |||
| raMax | double | deg | Max of ra | |||
| decMin | double | deg | Min of dec | |||
| decMax | double | deg | Max of dec | |||
| mu | double | deg | Survey mu of frame center | |||
| nu | double | deg | Survey nu of frame center | |||
| ra | double | deg | Ra of frame center | |||
| dec | double | deg | Dec of frame center | |||
| cx | double | Cartesian x of frame center | ||||
| cy | double | Cartesian y of frame center | ||||
| cz | double | Cartesian z of frame center | ||||
| htmID | long | The htmID for point at frame center | ||||
| img | int | The image in JPEG format |
The contraints for boundaries of the the different region
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| regionid | long | pointer to RegionDefs | ||||
| convexid | long | unique id for the convex | ||||
| x | double | x component of normal | ||||
| y | double | y component of normal | ||||
| z | double | z component of normal | ||||
| c | double | offset from center along normal |
Contains the detailed history of schema change
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| id | int | The unique key for entry | ||||
| filename | string | The name of the sql file | ||||
| date | string | Date of change | ||||
| name | string | Name of person making the change | ||||
| description | string | Detailed description of changes |
Table containing the definition of all indice
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| indexmapid | int | unique primary key for the indexmap | ||||
| code | string | one char designator of index category for lookup ('K'|'F'|'I') | ||||
| type | string | index type, one of ('primary key'|'foreign key'|'index'|'unique index') | ||||
| tableName | string | the name of the table the index is built on | ||||
| fieldList | string | the list of columns to be included in the index | ||||
| foreignKey | string | the definition of the foreign Key if any | ||||
| indexgroup | string | the group id, one of ('PHOTO'|'TAG'|'SPECTRO'|'QSO'|'META'|'TILES'|'FINISH') |
Contains the detailed inventory of database object
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| filename | string | The name of the sql file | ||||
| name | string | Name of DBObject | ||||
| type | string | Detailed description of changes |
Tracks the loading history of the databas
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| loadversion | int | |||||
| tstart | dateTime | |||||
| tend | dateTime | |||||
| dbname | string |
Contains a record describing the each mask objec
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| maskID | long | Unique Id number, composed of skyversion, rerun, run, camcol, field, filter, mask | ||||
| run | int | Run number | ||||
| rerun | int | Rerun number | ||||
| camcol | int | Camera column | ||||
| field | int | Field number | ||||
| mask | int | The object id within a field. Usually changes between reruns of the same field. | ||||
| filter | int | The enumerated filter [0..4] | ||||
| ra | double | deg | J2000 right ascension (r') | |||
| dec | double | deg | J2000 declination (r') | |||
| radius | double | deg | the radius of the bounding circle | |||
| area | string | Area descriptor for the mask object | ||||
| type | int | enumerated type of mask | ||||
| seeing | float | arcsecs | seeing width | |||
| cx | double | unit vector for ra+dec | ||||
| cy | double | unit vector for ra+dec | ||||
| cz | double | unit vector for ra+dec | ||||
| htmID | long | 20-deep hierarchical trangular mesh ID of this object |
Contains the objects inside a specific mas
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| objid | long | pointer to a PhotoObj | ||||
| maskID | long | Unique maskid | ||||
| maskType | int | enumerated type of mask |
Shows the names of partitions/filegroups and their relative size
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| fileGroupName | string | name of table or index | ||||
| size | float | size in GB/million objects | ||||
| comment | string | explanation |
The full photometric catalog quantities for SDSS imaging
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| objID | long | Unique SDSS identifier composed from [skyVersion,rerun,run,camcol,field,obj]. | ||||
| skyVersion | int | Layer of catalog (currently only one layer, 0; 0-15 available) | ||||
| run | int | Run number | ||||
| rerun | int | Rerun number | ||||
| camcol | int | Camera column | ||||
| field | int | Field number | ||||
| obj | int | The object id within a field. Usually changes between reruns of the same field | ||||
| mode | int | 1: primary, 2: secondary, 3: other | ||||
| nChild | int | Number of children if this is a composite object that has been deblended. BRIGHT (in a flags sense) objects also have nchild == 1, the non-BRIGHT sibling. | ||||
| type | int | Type classification of the object (star, galaxy, cosmic ray, etc.) | ||||
| clean | int | Clean photometry flag (1=clean, 0=unclean). | ||||
| probPSF | float | Probability that the object is a star. Currently 0 if type == 3 (galaxy), 1 if type == 6 (star). | ||||
| insideMask | int | Flag to indicate whether object is inside a mask and why | ||||
| flags | long | Photo Object Attribute Flags | ||||
| rowc | float | pix | Row center position (r-band coordinates) | |||
| rowcErr | float | pix | Row center position error (r-band coordinates) | |||
| colc | float | pix | Column center position (r-band coordinates) | |||
| colcErr | float | pix | Column center position error (r-band coordinates) | |||
| rowv | float | deg/day | Row-component of object's velocity | |||
| rowvErr | float | deg/day | Row-component of object's velocity error | |||
| colv | float | deg/day | Column-component of object's velocity | |||
| colvErr | float | deg/day | Column-component of object's velocity error | |||
| rowc_u | float | pix | Row center, u-band | |||
| rowc_g | float | pix | Row center, g-band | |||
| rowc_r | float | pix | Row center, r-band | |||
| rowc_i | float | pix | Row center, i-band | |||
| rowc_z | float | pix | Row center, z-band | |||
| rowcErr_u | float | pix | ERROR Row center error, u-band | |||
| rowcErr_g | float | pix | ERROR Row center error, g-band | |||
| rowcErr_r | float | pix | ERROR Row center error, r-band | |||
| rowcErr_i | float | pix | ERROR Row center error, i-band | |||
| rowcErr_z | float | pix | ERROR Row center error, z-band | |||
| colc_u | float | pix | Column center, u-band | |||
| colc_g | float | pix | Column center, g-band | |||
| colc_r | float | pix | Column center, r-band | |||
| colc_i | float | pix | Column center, i-band | |||
| colc_z | float | pix | Column center, z-band | |||
| colcErr_u | float | pix | Column center error, u-band | |||
| colcErr_g | float | pix | Column center error, g-band | |||
| colcErr_r | float | pix | Column center error, r-band | |||
| colcErr_i | float | pix | Column center error, i-band | |||
| colcErr_z | float | pix | Column center error, z-band | |||
| sky_u | float | nanomaggies/arcsec^2 | Sky flux at the center of object (allowing for siblings if blended). | |||
| sky_g | float | nanomaggies/arcsec^2 | Sky flux at the center of object (allowing for siblings if blended). | |||
| sky_r | float | nanomaggies/arcsec^2 | Sky flux at the center of object (allowing for siblings if blended). | |||
| sky_i | float | nanomaggies/arcsec^2 | Sky flux at the center of object (allowing for siblings if blended). | |||
| sky_z | float | nanomaggies/arcsec^2 | Sky flux at the center of object (allowing for siblings if blended). | |||
| skyIvar_u | float | nanomaggies/arcsec^2 | Sky flux inverse variance | |||
| skyIvar_g | float | nanomaggies/arcsec^2 | Sky flux inverse variance | |||
| skyIvar_r | float | nanomaggies/arcsec^2 | Sky flux inverse variance | |||
| skyIvar_i | float | nanomaggies/arcsec^2 | Sky flux inverse variance | |||
| skyIvar_z | float | nanomaggies/arcsec^2 | Sky flux inverse variance | |||
| psfMag_u | float | mag | PSF magnitude | |||
| psfMag_g | float | mag | PSF magnitude | |||
| psfMag_r | float | mag | PSF magnitude | |||
| psfMag_i | float | mag | PSF magnitude | |||
| psfMag_z | float | mag | PSF magnitude | |||
| psfMagErr_u | float | mag | PSF magnitude error | |||
| psfMagErr_g | float | mag | PSF magnitude error | |||
| psfMagErr_r | float | mag | PSF magnitude error | |||
| psfMagErr_i | float | mag | PSF magnitude error | |||
| psfMagErr_z | float | mag | PSF magnitude error | |||
| fiberMag_u | float | mag | Magnitude in 3 arcsec diameter fiber radius | |||
| fiberMag_g | float | mag | Magnitude in 3 arcsec diameter fiber radius | |||
| fiberMag_r | float | mag | Magnitude in 3 arcsec diameter fiber radius | |||
| fiberMag_i | float | mag | Magnitude in 3 arcsec diameter fiber radius | |||
| fiberMag_z | float | mag | Magnitude in 3 arcsec diameter fiber radius | |||
| fiberMagErr_u | float | mag | Error in magnitude in 3 arcsec diameter fiber radius | |||
| fiberMagErr_g | float | mag | Error in magnitude in 3 arcsec diameter fiber radius | |||
| fiberMagErr_r | float | mag | Error in magnitude in 3 arcsec diameter fiber radius | |||
| fiberMagErr_i | float | mag | Error in magnitude in 3 arcsec diameter fiber radius | |||
| fiberMagErr_z | float | mag | Error in magnitude in 3 arcsec diameter fiber radius | |||
| fiber2Mag_u | float | mag | Magnitude in 2 arcsec diameter fiber radius | |||
| fiber2Mag_g | float | mag | Magnitude in 2 arcsec diameter fiber radius | |||
| fiber2Mag_r | float | mag | Magnitude in 2 arcsec diameter fiber radius | |||
| fiber2Mag_i | float | mag | Magnitude in 2 arcsec diameter fiber radius | |||
| fiber2Mag_z | float | mag | Magnitude in 2 arcsec diameter fiber radius | |||
| fiber2MagErr_u | float | mag | Error in magnitude in 2 arcsec diameter fiber radius | |||
| fiber2MagErr_g | float | mag | Error in magnitude in 2 arcsec diameter fiber radius | |||
| fiber2MagErr_r | float | mag | Error in magnitude in 2 arcsec diameter fiber radius | |||
| fiber2MagErr_i | float | mag | Error in magnitude in 2 arcsec diameter fiber radius | |||
| fiber2MagErr_z | float | mag | Error in magnitude in 2 arcsec diameter fiber radius | |||
| petroMag_u | float | mag | Petrosian magnitude | |||
| petroMag_g | float | mag | Petrosian magnitude | |||
| petroMag_r | float | mag | Petrosian magnitude | |||
| petroMag_i | float | mag | Petrosian magnitude | |||
| petroMag_z | float | mag | Petrosian magnitude | |||
| petroMagErr_u | float | mag | Petrosian magnitude error | |||
| petroMagErr_g | float | mag | Petrosian magnitude error | |||
| petroMagErr_r | float | mag | Petrosian magnitude error | |||
| petroMagErr_i | float | mag | Petrosian magnitude error | |||
| petroMagErr_z | float | mag | Petrosian magnitude error | |||
| psfFlux_u | float | nanomaggies | PSF flux | |||
| psfFlux_g | float | nanomaggies | PSF flux | |||
| psfFlux_r | float | nanomaggies | PSF flux | |||
| psfFlux_i | float | nanomaggies | PSF flux | |||
| psfFlux_z | float | nanomaggies | PSF flux | |||
| psfFluxIvar_u | float | nanomaggies^{-2} | PSF flux inverse variance | |||
| psfFluxIvar_g | float | nanomaggies^{-2} | PSF flux inverse variance | |||
| psfFluxIvar_r | float | nanomaggies^{-2} | PSF flux inverse variance | |||
| psfFluxIvar_i | float | nanomaggies^{-2} | PSF flux inverse variance | |||
| psfFluxIvar_z | float | nanomaggies^{-2} | PSF flux inverse variance | |||
| fiberFlux_u | float | nanomaggies | Flux in 3 arcsec diameter fiber radius | |||
| fiberFlux_g | float | nanomaggies | Flux in 3 arcsec diameter fiber radius | |||
| fiberFlux_r | float | nanomaggies | Flux in 3 arcsec diameter fiber radius | |||
| fiberFlux_i | float | nanomaggies | Flux in 3 arcsec diameter fiber radius | |||
| fiberFlux_z | float | nanomaggies | Flux in 3 arcsec diameter fiber radius | |||
| fiberFluxIvar_u | float | nanomaggies^{-2} | Inverse variance in flux in 3 arcsec diameter fiber radius | |||
| fiberFluxIvar_g | float | nanomaggies^{-2} | Inverse variance in flux in 3 arcsec diameter fiber radius | |||
| fiberFluxIvar_r | float | nanomaggies^{-2} | Inverse variance in flux in 3 arcsec diameter fiber radius | |||
| fiberFluxIvar_i | float | nanomaggies^{-2} | Inverse variance in flux in 3 arcsec diameter fiber radius | |||
| fiberFluxIvar_z | float | nanomaggies^{-2} | Inverse variance in flux in 3 arcsec diameter fiber radius | |||
| fiber2Flux_u | float | nanomaggies | Flux in 2 arcsec diameter fiber radius | |||
| fiber2Flux_g | float | nanomaggies | Flux in 2 arcsec diameter fiber radius | |||
| fiber2Flux_r | float | nanomaggies | Flux in 2 arcsec diameter fiber radius | |||
| fiber2Flux_i | float | nanomaggies | Flux in 2 arcsec diameter fiber radius | |||
| fiber2Flux_z | float | nanomaggies | Flux in 2 arcsec diameter fiber radius | |||
| fiber2FluxIvar_u | float | nanomaggies^{-2} | Inverse variance in flux in 2 arcsec diameter fiber radius | |||
| fiber2FluxIvar_g | float | nanomaggies^{-2} | Inverse variance in flux in 2 arcsec diameter fiber radius | |||
| fiber2FluxIvar_r | float | nanomaggies^{-2} | Inverse variance in flux in 2 arcsec diameter fiber radius | |||
| fiber2FluxIvar_i | float | nanomaggies^{-2} | Inverse variance in flux in 2 arcsec diameter fiber radius | |||
| fiber2FluxIvar_z | float | nanomaggies^{-2} | Inverse variance in flux in 2 arcsec diameter fiber radius | |||
| petroFlux_u | float | nanomaggies | Petrosian flux | |||
| petroFlux_g | float | nanomaggies | Petrosian flux | |||
| petroFlux_r | float | nanomaggies | Petrosian flux | |||
| petroFlux_i | float | nanomaggies | Petrosian flux | |||
| petroFlux_z | float | nanomaggies | Petrosian flux | |||
| petroFluxIvar_u | float | nanomaggies^{-2} | Petrosian flux inverse variance | |||
| petroFluxIvar_g | float | nanomaggies^{-2} | Petrosian flux inverse variance | |||
| petroFluxIvar_r | float | nanomaggies^{-2} | Petrosian flux inverse variance | |||
| petroFluxIvar_i | float | nanomaggies^{-2} | Petrosian flux inverse variance | |||
| petroFluxIvar_z | float | nanomaggies^{-2} | Petrosian flux inverse variance | |||
| petroRad_u | float | arcsec | Petrosian radius | |||
| petroRad_g | float | arcsec | Petrosian radius | |||
| petroRad_r | float | arcsec | Petrosian radius | |||
| petroRad_i | float | arcsec | Petrosian radius | |||
| petroRad_z | float | arcsec | Petrosian radius | |||
| petroRadErr_u | float | arcsec | Petrosian radius error | |||
| petroRadErr_g | float | arcsec | Petrosian radius error | |||
| petroRadErr_r | float | arcsec | Petrosian radius error | |||
| petroRadErr_i | float | arcsec | Petrosian radius error | |||
| petroRadErr_z | float | arcsec | Petrosian radius error | |||
| petroR50_u | float | arcsec | Radius containing 50% of Petrosian flux | |||
| petroR50_g | float | arcsec | Radius containing 50% of Petrosian flux | |||
| petroR50_r | float | arcsec | Radius containing 50% of Petrosian flux | |||
| petroR50_i | float | arcsec | Radius containing 50% of Petrosian flux | |||
| petroR50_z | float | arcsec | Radius containing 50% of Petrosian flux | |||
| petroR50Err_u | float | arcsec | Error in radius with 50% of Petrosian flux error | |||
| petroR50Err_g | float | arcsec | Error in radius with 50% of Petrosian flux error | |||
| petroR50Err_r | float | arcsec | Error in radius with 50% of Petrosian flux error | |||
| petroR50Err_i | float | arcsec | Error in radius with 50% of Petrosian flux error | |||
| petroR50Err_z | float | arcsec | Error in radius with 50% of Petrosian flux error | |||
| petroR90_u | float | arcsec | Radius containing 90% of Petrosian flux | |||
| petroR90_g | float | arcsec | Radius containing 90% of Petrosian flux | |||
| petroR90_r | float | arcsec | Radius containing 90% of Petrosian flux | |||
| petroR90_i | float | arcsec | Radius containing 90% of Petrosian flux | |||
| petroR90_z | float | arcsec | Radius containing 90% of Petrosian flux | |||
| petroR90Err_u | float | arcsec | Error in radius with 90% of Petrosian flux error | |||
| petroR90Err_g | float | arcsec | Error in radius with 90% of Petrosian flux error | |||
| petroR90Err_r | float | arcsec | Error in radius with 90% of Petrosian flux error | |||
| petroR90Err_i | float | arcsec | Error in radius with 90% of Petrosian flux error | |||
| petroR90Err_z | float | arcsec | Error in radius with 90% of Petrosian flux error | |||
| q_u | float | Stokes Q parameter | ||||
| q_g | float | Stokes Q parameter | ||||
| q_r | float | Stokes Q parameter | ||||
| q_i | float | Stokes Q parameter | ||||
| q_z | float | Stokes Q parameter | ||||
| qErr_u | float | Stokes Q parameter error | ||||
| qErr_g | float | Stokes Q parameter error | ||||
| qErr_r | float | Stokes Q parameter error | ||||
| qErr_i | float | Stokes Q parameter error | ||||
| qErr_z | float | Stokes Q parameter error | ||||
| u_u | float | Stokes U parameter | ||||
| u_g | float | Stokes U parameter | ||||
| u_r | float | Stokes U parameter | ||||
| u_i | float | Stokes U parameter | ||||
| u_z | float | Stokes U parameter | ||||
| uErr_u | float | Stokes U parameter error | ||||
| uErr_g | float | Stokes U parameter error | ||||
| uErr_r | float | Stokes U parameter error | ||||
| uErr_i | float | Stokes U parameter error | ||||
| uErr_z | float | Stokes U parameter error | ||||
| mE1_u | float | Adaptive E1 shape measure (pixel coordinates) | ||||
| mE1_g | float | Adaptive E1 shape measure (pixel coordinates) | ||||
| mE1_r | float | Adaptive E1 shape measure (pixel coordinates) | ||||
| mE1_i | float | Adaptive E1 shape measure (pixel coordinates) | ||||
| mE1_z | float | Adaptive E1 shape measure (pixel coordinates) | ||||
| mE2_u | float | Adaptive E2 shape measure (pixel coordinates) | ||||
| mE2_g | float | Adaptive E2 shape measure (pixel coordinates) | ||||
| mE2_r | float | Adaptive E2 shape measure (pixel coordinates) | ||||
| mE2_i | float | Adaptive E2 shape measure (pixel coordinates) | ||||
| mE2_z | float | Adaptive E2 shape measure (pixel coordinates) | ||||
| mE1E1Err_u | float | Covariance in E1/E1 shape measure (pixel coordinates) | ||||
| mE1E1Err_g | float | Covariance in E1/E1 shape measure (pixel coordinates) | ||||
| mE1E1Err_r | float | Covariance in E1/E1 shape measure (pixel coordinates) | ||||
| mE1E1Err_i | float | Covariance in E1/E1 shape measure (pixel coordinates) | ||||
| mE1E1Err_z | float | Covariance in E1/E1 shape measure (pixel coordinates) | ||||
| mE1E2Err_u | float | Covariance in E1/E2 shape measure (pixel coordinates) | ||||
| mE1E2Err_g | float | Covariance in E1/E2 shape measure (pixel coordinates) | ||||
| mE1E2Err_r | float | Covariance in E1/E2 shape measure (pixel coordinates) | ||||
| mE1E2Err_i | float | Covariance in E1/E2 shape measure (pixel coordinates) | ||||
| mE1E2Err_z | float | Covariance in E1/E2 shape measure (pixel coordinates) | ||||
| mE2E2Err_u | float | Covariance in E2/E2 shape measure (pixel coordinates) | ||||
| mE2E2Err_g | float | Covariance in E2/E2 shape measure (pixel coordinates) | ||||
| mE2E2Err_r | float | Covariance in E2/E2 shape measure (pixel coordinates) | ||||
| mE2E2Err_i | float | Covariance in E2/E2 shape measure (pixel coordinates) | ||||
| mE2E2Err_z | float | Covariance in E2/E2 shape measure (pixel coordinates) | ||||
| mRrCc_u | float | Adaptive ( + ) (pixel coordinates) | ||||
| mRrCc_g | float | Adaptive ( + ) (pixel coordinates) | ||||
| mRrCc_r | float | Adaptive ( + ) (pixel coordinates) | ||||
| mRrCc_i | float | Adaptive ( + ) (pixel coordinates) | ||||
| mRrCc_z | float | Adaptive ( + ) (pixel coordinates) | ||||
| mRrCcErr_u | float | Error in adaptive ( + ) (pixel coordinates) | ||||
| mRrCcErr_g | float | Error in adaptive ( + ) (pixel coordinates) | ||||
| mRrCcErr_r | float | Error in adaptive ( + ) (pixel coordinates) | ||||
| mRrCcErr_i | float | Error in adaptive ( + ) (pixel coordinates) | ||||
| mRrCcErr_z | float | Error in adaptive ( + ) (pixel coordinates) | ||||
| mCr4_u | float | Adaptive fourth moment of object (pixel coordinates) | ||||
| mCr4_g | float | Adaptive fourth moment of object (pixel coordinates) | ||||
| mCr4_r | float | Adaptive fourth moment of object (pixel coordinates) | ||||
| mCr4_i | float | Adaptive fourth moment of object (pixel coordinates) | ||||
| mCr4_z | float | Adaptive fourth moment of object (pixel coordinates) | ||||
| mE1PSF_u | float | Adaptive E1 for PSF (pixel coordinates) | ||||
| mE1PSF_g | float | Adaptive E1 for PSF (pixel coordinates) | ||||
| mE1PSF_r | float | Adaptive E1 for PSF (pixel coordinates) | ||||
| mE1PSF_i | float | Adaptive E1 for PSF (pixel coordinates) | ||||
| mE1PSF_z | float | Adaptive E1 for PSF (pixel coordinates) | ||||
| mE2PSF_u | float | Adaptive E2 for PSF (pixel coordinates) | ||||
| mE2PSF_g | float | Adaptive E2 for PSF (pixel coordinates) | ||||
| mE2PSF_r | float | Adaptive E2 for PSF (pixel coordinates) | ||||
| mE2PSF_i | float | Adaptive E2 for PSF (pixel coordinates) | ||||
| mE2PSF_z | float | Adaptive E2 for PSF (pixel coordinates) | ||||
| mRrCcPSF_u | float | Adaptive ( + ) for PSF (pixel coordinates) | ||||
| mRrCcPSF_g | float | Adaptive ( + ) for PSF (pixel coordinates) | ||||
| mRrCcPSF_r | float | Adaptive ( + ) for PSF (pixel coordinates) | ||||
| mRrCcPSF_i | float | Adaptive ( + ) for PSF (pixel coordinates) | ||||
| mRrCcPSF_z | float | Adaptive ( + ) for PSF (pixel coordinates) | ||||
| mCr4PSF_u | float | Adaptive fourth moment for PSF (pixel coordinates) | ||||
| mCr4PSF_g | float | Adaptive fourth moment for PSF (pixel coordinates) | ||||
| mCr4PSF_r | float | Adaptive fourth moment for PSF (pixel coordinates) | ||||
| mCr4PSF_i | float | Adaptive fourth moment for PSF (pixel coordinates) | ||||
| mCr4PSF_z | float | Adaptive fourth moment for PSF (pixel coordinates) | ||||
| deVRad_u | float | arcsec | de Vaucouleurs fit scale radius | |||
| deVRad_g | float | arcsec | de Vaucouleurs fit scale radius | |||
| deVRad_r | float | arcsec | de Vaucouleurs fit scale radius | |||
| deVRad_i | float | arcsec | de Vaucouleurs fit scale radius | |||
| deVRad_z | float | arcsec | de Vaucouleurs fit scale radius | |||
| deVRadErr_u | float | arcsec | Error in de Vaucouleurs fit scale radius error | |||
| deVRadErr_g | float | arcsec | Error in de Vaucouleurs fit scale radius error | |||
| deVRadErr_r | float | arcsec | Error in de Vaucouleurs fit scale radius error | |||
| deVRadErr_i | float | arcsec | Error in de Vaucouleurs fit scale radius error | |||
| deVRadErr_z | float | arcsec | Error in de Vaucouleurs fit scale radius error | |||
| deVAB_u | float | de Vaucouleurs fit b/a | ||||
| deVAB_g | float | de Vaucouleurs fit b/a | ||||
| deVAB_r | float | de Vaucouleurs fit b/a | ||||
| deVAB_i | float | de Vaucouleurs fit b/a | ||||
| deVAB_z | float | de Vaucouleurs fit b/a | ||||
| deVABErr_u | float | de Vaucouleurs fit b/a error | ||||
| deVABErr_g | float | de Vaucouleurs fit b/a error | ||||
| deVABErr_r | float | de Vaucouleurs fit b/a error | ||||
| deVABErr_i | float | de Vaucouleurs fit b/a error | ||||
| deVABErr_z | float | de Vaucouleurs fit b/a error | ||||
| deVPhi_u | float | de Vaucouleurs fit position angle (+N thru E) | deg | |||
| deVPhi_g | float | de Vaucouleurs fit position angle (+N thru E) | deg | |||
| deVPhi_r | float | de Vaucouleurs fit position angle (+N thru E) | deg | |||
| deVPhi_i | float | de Vaucouleurs fit position angle (+N thru E) | deg | |||
| deVPhi_z | float | de Vaucouleurs fit position angle (+N thru E) | deg | |||
| deVMag_u | float | de Vaucouleurs magnitude fit | mag | |||
| deVMag_g | float | de Vaucouleurs magnitude fit | mag | |||
| deVMag_r | float | de Vaucouleurs magnitude fit | mag | |||
| deVMag_i | float | de Vaucouleurs magnitude fit | mag | |||
| deVMag_z | float | de Vaucouleurs magnitude fit | mag | |||
| deVMagErr_u | float | de Vaucouleurs magnitude fit error | mag | |||
| deVMagErr_g | float | de Vaucouleurs magnitude fit error | mag | |||
| deVMagErr_r | float | de Vaucouleurs magnitude fit error | mag | |||
| deVMagErr_i | float | de Vaucouleurs magnitude fit error | mag | |||
| deVMagErr_z | float | de Vaucouleurs magnitude fit error | mag | |||
| deVFlux_u | float | de Vaucouleurs magnitude fit | nanomaggies | |||
| deVFlux_g | float | de Vaucouleurs magnitude fit | nanomaggies | |||
| deVFlux_r | float | de Vaucouleurs magnitude fit | nanomaggies | |||
| deVFlux_i | float | de Vaucouleurs magnitude fit | nanomaggies | |||
| deVFlux_z | float | de Vaucouleurs magnitude fit | nanomaggies | |||
| deVFluxIvar_u | float | de Vaucouleurs magnitude fit inverse variance | nanomaggies^{-2} | |||
| deVFluxIvar_g | float | de Vaucouleurs magnitude fit inverse variance | nanomaggies^{-2} | |||
| deVFluxIvar_r | float | de Vaucouleurs magnitude fit inverse variance | nanomaggies^{-2} | |||
| deVFluxIvar_i | float | de Vaucouleurs magnitude fit inverse variance | nanomaggies^{-2} | |||
| deVFluxIvar_z | float | de Vaucouleurs magnitude fit inverse variance | nanomaggies^{-2} | |||
| expRad_u | float | arcsec | Exponential fit scale radius | |||
| expRad_g | float | arcsec | Exponential fit scale radius | |||
| expRad_r | float | arcsec | Exponential fit scale radius | |||
| expRad_i | float | arcsec | Exponential fit scale radius | |||
| expRad_z | float | arcsec | Exponential fit scale radius | |||
| expRadErr_u | float | arcsec | Exponential fit scale radius error | |||
| expRadErr_g | float | arcsec | Exponential fit scale radius error | |||
| expRadErr_r | float | arcsec | Exponential fit scale radius error | |||
| expRadErr_i | float | arcsec | Exponential fit scale radius error | |||
| expRadErr_z | float | arcsec | Exponential fit scale radius error | |||
| expAB_u | float | Exponential fit b/a | ||||
| expAB_g | float | Exponential fit b/a | ||||
| expAB_r | float | Exponential fit b/a | ||||
| expAB_i | float | Exponential fit b/a | ||||
| expAB_z | float | Exponential fit b/a | ||||
| expABErr_u | float | Exponential fit b/a | ||||
| expABErr_g | float | Exponential fit b/a | ||||
| expABErr_r | float | Exponential fit b/a | ||||
| expABErr_i | float | Exponential fit b/a | ||||
| expABErr_z | float | Exponential fit b/a | ||||
| expPhi_u | float | deg | Exponential fit position angle (+N thru E) | |||
| expPhi_g | float | deg | Exponential fit position angle (+N thru E) | |||
| expPhi_r | float | deg | Exponential fit position angle (+N thru E) | |||
| expPhi_i | float | deg | Exponential fit position angle (+N thru E) | |||
| expPhi_z | float | deg | Exponential fit position angle (+N thru E) | |||
| expMag_u | float | mag | Exponential fit magnitude | |||
| expMag_g | float | mag | Exponential fit magnitude | |||
| expMag_r | float | mag | Exponential fit magnitude | |||
| expMag_i | float | mag | Exponential fit magnitude | |||
| expMag_z | float | mag | Exponential fit magnitude | |||
| expMagErr_u | float | mag | Exponential fit magnitude error | |||
| expMagErr_g | float | mag | Exponential fit magnitude error | |||
| expMagErr_r | float | mag | Exponential fit magnitude error | |||
| expMagErr_i | float | mag | Exponential fit magnitude error | |||
| expMagErr_z | float | mag | Exponential fit magnitude error | |||
| modelMag_u | float | mag | better of DeV/Exp magnitude fit | |||
| modelMag_g | float | mag | better of DeV/Exp magnitude fit | |||
| modelMag_r | float | mag | better of DeV/Exp magnitude fit | |||
| modelMag_i | float | mag | better of DeV/Exp magnitude fit | |||
| modelMag_z | float | mag | better of DeV/Exp magnitude fit | |||
| modelMagErr_u | float | mag | Error in better of DeV/Exp magnitude fit | |||
| modelMagErr_g | float | mag | Error in better of DeV/Exp magnitude fit | |||
| modelMagErr_r | float | mag | Error in better of DeV/Exp magnitude fit | |||
| modelMagErr_i | float | mag | Error in better of DeV/Exp magnitude fit | |||
| modelMagErr_z | float | mag | Error in better of DeV/Exp magnitude fit | |||
| cModelMag_u | float | mag | DeV+Exp magnitude | |||
| cModelMag_g | float | mag | DeV+Exp magnitude | |||
| cModelMag_r | float | mag | DeV+Exp magnitude | |||
| cModelMag_i | float | mag | DeV+Exp magnitude | |||
| cModelMag_z | float | mag | DeV+Exp magnitude | |||
| cModelMagErr_u | float | mag | DeV+Exp magnitude error | |||
| cModelMagErr_g | float | mag | DeV+Exp magnitude error | |||
| cModelMagErr_r | float | mag | DeV+Exp magnitude error | |||
| cModelMagErr_i | float | mag | DeV+Exp magnitude error | |||
| cModelMagErr_z | float | mag | DeV+Exp magnitude error | |||
| expFlux_u | float | nanomaggies | Exponential fit flux | |||
| expFlux_g | float | nanomaggies | Exponential fit flux | |||
| expFlux_r | float | nanomaggies | Exponential fit flux | |||
| expFlux_i | float | nanomaggies | Exponential fit flux | |||
| expFlux_z | float | nanomaggies | Exponential fit flux | |||
| expFluxIvar_u | float | nanomaggies^{-2} | Exponential fit flux inverse variance | |||
| expFluxIvar_g | float | nanomaggies^{-2} | Exponential fit flux inverse variance | |||
| expFluxIvar_r | float | nanomaggies^{-2} | Exponential fit flux inverse variance | |||
| expFluxIvar_i | float | nanomaggies^{-2} | Exponential fit flux inverse variance | |||
| expFluxIvar_z | float | nanomaggies^{-2} | Exponential fit flux inverse variance | |||
| modelFlux_u | float | nanomaggies | better of DeV/Exp flux fit | |||
| modelFlux_g | float | nanomaggies | better of DeV/Exp flux fit | |||
| modelFlux_r | float | nanomaggies | better of DeV/Exp flux fit | |||
| modelFlux_i | float | nanomaggies | better of DeV/Exp flux fit | |||
| modelFlux_z | float | nanomaggies | better of DeV/Exp flux fit | |||
| modelFluxIvar_u | float | nanomaggies^{-2} | Inverse variance in better of DeV/Exp flux fit | |||
| modelFluxIvar_g | float | nanomaggies^{-2} | Inverse variance in better of DeV/Exp flux fit | |||
| modelFluxIvar_r | float | nanomaggies^{-2} | Inverse variance in better of DeV/Exp flux fit | |||
| modelFluxIvar_i | float | nanomaggies^{-2} | Inverse variance in better of DeV/Exp flux fit | |||
| modelFluxIvar_z | float | nanomaggies^{-2} | Inverse variance in better of DeV/Exp flux fit | |||
| cModelFlux_u | float | nanomaggies | better of DeV+Exp flux | |||
| cModelFlux_g | float | nanomaggies | better of DeV+Exp flux | |||
| cModelFlux_r | float | nanomaggies | better of DeV+Exp flux | |||
| cModelFlux_i | float | nanomaggies | better of DeV+Exp flux | |||
| cModelFlux_z | float | nanomaggies | better of DeV+Exp flux | |||
| cModelFluxIvar_u | float | nanomaggies^{-2} | Inverse variance in DeV+Exp flux fit | |||
| cModelFluxIvar_g | float | nanomaggies^{-2} | Inverse variance in DeV+Exp flux fit | |||
| cModelFluxIvar_r | float | nanomaggies^{-2} | Inverse variance in DeV+Exp flux fit | |||
| cModelFluxIvar_i | float | nanomaggies^{-2} | Inverse variance in DeV+Exp flux fit | |||
| cModelFluxIvar_z | float | nanomaggies^{-2} | Inverse variance in DeV+Exp flux fit | |||
| aperFlux7_u | float | nanomaggies | Aperture flux within 7.3 arcsec | |||
| aperFlux7_g | float | nanomaggies | Aperture flux within 7.3 arcsec | |||
| aperFlux7_r | float | nanomaggies | Aperture flux within 7.3 arcsec | |||
| aperFlux7_i | float | nanomaggies | Aperture flux within 7.3 arcsec | |||
| aperFlux7_z | float | nanomaggies | Aperture flux within 7.3 arcsec | |||
| aperFlux7Ivar_u | float | nanomaggies^{-2} | Inverse variance of aperture flux within 7.3 arcsec | |||
| aperFlux7Ivar_g | float | nanomaggies^{-2} | Inverse variance of aperture flux within 7.3 arcsec | |||
| aperFlux7Ivar_r | float | nanomaggies^{-2} | Inverse variance of aperture flux within 7.3 arcsec | |||
| aperFlux7Ivar_i | float | nanomaggies^{-2} | Inverse variance of aperture flux within 7.3 arcsec | |||
| aperFlux7Ivar_z | float | nanomaggies^{-2} | Inverse variance of aperture flux within 7.3 arcsec | |||
| lnLStar_u | float | Star ln(likelihood) | ||||
| lnLStar_g | float | Star ln(likelihood) | ||||
| lnLStar_r | float | Star ln(likelihood) | ||||
| lnLStar_i | float | Star ln(likelihood) | ||||
| lnLStar_z | float | Star ln(likelihood) | ||||
| lnLExp_u | float | Exponential disk fit ln(likelihood) | ||||
| lnLExp_g | float | Exponential disk fit ln(likelihood) | ||||
| lnLExp_r | float | Exponential disk fit ln(likelihood) | ||||
| lnLExp_i | float | Exponential disk fit ln(likelihood) | ||||
| lnLExp_z | float | Exponential disk fit ln(likelihood) | ||||
| lnLDeV_u | float | de Vaucouleurs fit ln(likelihood) | ||||
| lnLDeV_g | float | de Vaucouleurs fit ln(likelihood) | ||||
| lnLDeV_r | float | de Vaucouleurs fit ln(likelihood) | ||||
| lnLDeV_i | float | de Vaucouleurs fit ln(likelihood) | ||||
| lnLDeV_z | float | de Vaucouleurs fit ln(likelihood) | ||||
| fracDeV_u | float | Weight of deV component in deV+Exp model | ||||
| fracDeV_g | float | Weight of deV component in deV+Exp model | ||||
| fracDeV_r | float | Weight of deV component in deV+Exp model | ||||
| fracDeV_i | float | Weight of deV component in deV+Exp model | ||||
| fracDeV_z | float | Weight of deV component in deV+Exp model | ||||
| flags_u | long | Object detection flags per band | ||||
| flags_g | long | Object detection flags per band | ||||
| flags_r | long | Object detection flags per band | ||||
| flags_i | long | Object detection flags per band | ||||
| flags_z | long | Object detection flags per band | ||||
| type_u | int | Object type classification per band | ||||
| type_g | int | Object type classification per band | ||||
| type_r | int | Object type classification per band | ||||
| type_i | int | Object type classification per band | ||||
| type_z | int | Object type classification per band | ||||
| probPSF_u | float | Probablity object is a star in each filter. | ||||
| probPSF_g | float | Probablity object is a star in each filter. | ||||
| probPSF_r | float | Probablity object is a star in each filter. | ||||
| probPSF_i | float | Probablity object is a star in each filter. | ||||
| probPSF_z | float | Probablity object is a star in each filter. | ||||
| ra | double | deg | J2000 Right Ascension (r-band) | |||
| dec | double | deg | J2000 Declination (r-band) | |||
| cx | double | unit vector for ra+dec | ||||
| cy | double | unit vector for ra+dec | ||||
| cz | double | unit vector for ra+dec | ||||
| raErr | double | arcsec | Error in RA (* cos(Dec), that is, proper units) | |||
| decErr | double | arcsec | Error in Dec | |||
| b | double | deg | Galactic latitude | |||
| l | double | deg | Galactic longitude | |||
| offsetRa_u | float | arcsec | filter position RA minus final RA (* cos(Dec), that is, proper units) | |||
| offsetRa_g | float | arcsec | filter position RA minus final RA (* cos(Dec), that is, proper units) | |||
| offsetRa_r | float | arcsec | filter position RA minus final RA (* cos(Dec), that is, proper units) | |||
| offsetRa_i | float | arcsec | filter position RA minus final RA (* cos(Dec), that is, proper units) | |||
| offsetRa_z | float | arcsec | filter position RA minus final RA (* cos(Dec), that is, proper units) | |||
| offsetDec_u | float | arcsec | filter position Dec minus final Dec | |||
| offsetDec_g | float | arcsec | filter position Dec minus final Dec | |||
| offsetDec_r | float | arcsec | filter position Dec minus final Dec | |||
| offsetDec_i | float | arcsec | filter position Dec minus final Dec | |||
| offsetDec_z | float | arcsec | filter position Dec minus final Dec | |||
| extinction_u | float | mag | Extinction in u-band | |||
| extinction_g | float | mag | Extinction in g-band | |||
| extinction_r | float | mag | Extinction in r-band | |||
| extinction_i | float | mag | Extinction in i-band | |||
| extinction_z | float | mag | Extinction in z-band | |||
| psffwhm_u | float | arcsec | FWHM in u-band | |||
| psffwhm_g | float | arcsec | FWHM in g-band | |||
| psffwhm_r | float | arcsec | FWHM in r-band | |||
| psffwhm_i | float | arcsec | FWHM in i-band | |||
| psffwhm_z | float | arcsec | FWHM in z-band | |||
| mjd | int | days | Date of observation | |||
| airmass_u | float | Airmass at time of observation in u-band | ||||
| airmass_g | float | Airmass at time of observation in g-band | ||||
| airmass_r | float | Airmass at time of observation in r-band | ||||
| airmass_i | float | Airmass at time of observation in i-band | ||||
| airmass_z | float | Airmass at time of observation in z-band | ||||
| phioffset_u | float | deg | Degrees to add to CCD-aligned angle to convert to E of N | |||
| phioffset_g | float | deg | Degrees to add to CCD-aligned angle to convert to E of N | |||
| phioffset_r | float | deg | Degrees to add to CCD-aligned angle to convert to E of N | |||
| phioffset_i | float | deg | Degrees to add to CCD-aligned angle to convert to E of N | |||
| phioffset_z | float | deg | Degrees to add to CCD-aligned angle to convert to E of N | |||
| nProf_u | int | Number of Profile Bins | ||||
| nProf_g | int | Number of Profile Bins | ||||
| nProf_r | int | Number of Profile Bins | ||||
| nProf_i | int | Number of Profile Bins | ||||
| nProf_z | int | Number of Profile Bins | ||||
| loadVersion | int | Load Version | ||||
| htmID | long | 20-deep hierarchical trangular mesh ID of this object | ||||
| fieldID | long | Link to the field this object is in | ||||
| parentID | long | Pointer to parent (if object deblended) or BRIGHT detection (if object has one), else 0 | ||||
| specObjID | long | Pointer to the spectrum of object, if exists, else 0 | ||||
| u | float | mag | Shorthand alias for modelMag | |||
| g | float | mag | Shorthand alias for modelMag | |||
| r | float | mag | Shorthand alias for modelMag | |||
| i | float | mag | Shorthand alias for modelMag | |||
| z | float | mag | Shorthand alias for modelMag | |||
| err_u | float | mag | Error in modelMag alias | |||
| err_g | float | mag | Error in modelMag alias | |||
| err_r | float | mag | Error in modelMag alias | |||
| err_i | float | mag | Error in modelMag alias | |||
| err_z | float | mag | Error in modelMag alias | |||
| dered_u | float | mag | Simplified mag, corrected for extinction: modelMag-extinction | |||
| dered_g | float | mag | Simplified mag, corrected for extinction: modelMag-extinction | |||
| dered_r | float | mag | Simplified mag, corrected for extinction: modelMag-extinction | |||
| dered_i | float | mag | Simplified mag, corrected for extinction: modelMag-extinction | |||
| dered_z | float | mag | Simplified mag, corrected for extinction: modelMag-extinction | |||
| cloudCam_u | int | Cloud camera status for observation in u-band | ||||
| cloudCam_g | int | Cloud camera status for observation in g-band | ||||
| cloudCam_r | int | Cloud camera status for observation in r-band | ||||
| cloudCam_i | int | Cloud camera status for observation in i-band | ||||
| cloudCam_z | int | Cloud camera status for observation in z-band | ||||
| resolveStatus | int | Resolve status of object | ||||
| thingId | int | Unique identifier from global resolve | ||||
| balkanId | int | What balkan object is in from window | ||||
| nObserve | int | Number of observations of this object | ||||
| nDetect | int | Number of detections of this object | ||||
| nEdge | int | Number of observations of this object near an edge | ||||
| score | float | Quality of field (0-1) | ||||
| calibStatus_u | int | Calibration status in u-band | ||||
| calibStatus_g | int | Calibration status in g-band | ||||
| calibStatus_r | int | Calibration status in r-band | ||||
| calibStatus_i | int | Calibration status in i-band | ||||
| calibStatus_z | int | Calibration status in z-band | ||||
| nMgyPerCount_u | float | nmgy/count | nanomaggies per count in u-band | |||
| nMgyPerCount_g | float | nmgy/count | nanomaggies per count in g-band | |||
| nMgyPerCount_r | float | nmgy/count | nanomaggies per count in r-band | |||
| nMgyPerCount_i | float | nmgy/count | nanomaggies per count in i-band | |||
| nMgyPerCount_z | float | nmgy/count | nanomaggies per count in z-band | |||
| TAI_u | double | sec | time of observation (TAI) in each filter | |||
| TAI_g | double | sec | time of observation (TAI) in each filter | |||
| TAI_r | double | sec | time of observation (TAI) in each filter | |||
| TAI_i | double | sec | time of observation (TAI) in each filter | |||
| TAI_z | double | sec | time of observation (TAI) in each filter |
Contains the spatial cross-match between DR8 photoobj and DR7 photoobj
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| dr7objID | long | Unique DR7 identifier composed from [skyVersion,rerun,run,camcol,field,obj]. | ||||
| dr8objID | long | Unique DR8 identifier composed from [skyVersion,rerun,run,camcol,field,obj]. | ||||
| distance | double | Distance in arcmin between the DR7 and DR8 positions | ||||
| modeDR7 | int | DR7 mode, 1: primary, 2: secondary, 3: family object. | ||||
| modeDR8 | int | DR8 mode, 1: primary, 2: secondary, 3: family object. | ||||
| skyVersion | int | 0 = OPDB target, 1 = OPDB best | ||||
| run | int | Run number | ||||
| rerun | int | Rerun number | ||||
| camcol | int | Camera column | ||||
| field | int | Field number | ||||
| obj | int | The object id within a field. Usually changes between reruns of the same field. | ||||
| nChild | int | Number of children if this is a composite object that has been deblended. BRIGHT (in a flags sense) objects also have nchild == 1, the non-BRIGHT sibling. | ||||
| type | int | Morphological type classification of the object. | ||||
| probPSF | float | Probability that the object is a star. Currently 0 if type == 3 (galaxy), 1 if type == 6 (star). | ||||
| insideMask | int | Flag to indicate whether object is inside a mask and why | ||||
| flags | long | Photo Object Attribute Flags | ||||
| psfMag_u | float | mag | PSF flux | |||
| psfMag_g | float | mag | PSF flux | |||
| psfMag_r | float | mag | PSF flux | |||
| psfMag_i | float | mag | PSF flux | |||
| psfMag_z | float | mag | PSF flux | |||
| psfMagErr_u | float | mag | PSF flux error | |||
| psfMagErr_g | float | mag | PSF flux error | |||
| psfMagErr_r | float | mag | PSF flux error | |||
| psfMagErr_i | float | mag | PSF flux error | |||
| psfMagErr_z | float | mag | PSF flux error | |||
| petroMag_u | float | mag | Petrosian flux | |||
| petroMag_g | float | mag | Petrosian flux | |||
| petroMag_r | float | mag | Petrosian flux | |||
| petroMag_i | float | mag | Petrosian flux | |||
| petroMag_z | float | mag | Petrosian flux | |||
| petroMagErr_u | float | mag | Petrosian flux error | |||
| petroMagErr_g | float | mag | Petrosian flux error | |||
| petroMagErr_r | float | mag | Petrosian flux error | |||
| petroMagErr_i | float | mag | Petrosian flux error | |||
| petroMagErr_z | float | mag | Petrosian flux error | |||
| petroR50_r | float | arcsec | Radius containing 50% of Petrosian flux | |||
| petroR90_r | float | arcsec | Radius containing 90% of Petrosian flux | |||
| modelMag_u | float | mag | better of DeV/Exp magnitude fit | |||
| modelMag_g | float | mag | better of DeV/Exp magnitude fit | |||
| modelMag_r | float | mag | better of DeV/Exp magnitude fit | |||
| modelMag_i | float | mag | better of DeV/Exp magnitude fit | |||
| modelMag_z | float | mag | better of DeV/Exp magnitude fit | |||
| modelMagErr_u | float | mag | better of DeV/Exp magnitude fit error | |||
| modelMagErr_g | float | mag | better of DeV/Exp magnitude fit error | |||
| modelMagErr_r | float | mag | better of DeV/Exp magnitude fit error | |||
| modelMagErr_i | float | mag | better of DeV/Exp magnitude fit error | |||
| modelMagErr_z | float | mag | better of DeV/Exp magnitude fit error | |||
| mRrCc_r | float | Adaptive (<r^2> + <c^2>) | ||||
| mRrCcErr_r | float | Error in adaptive (<r^2> + <c^2>) | ||||
| lnLStar_r | float | Star ln(likelihood) | ||||
| lnLExp_r | float | Exponential disk fit ln(likelihood) | ||||
| lnLDeV_r | float | DeVaucouleurs fit ln(likelihood) | ||||
| status | int | Status of the object in the survey | ||||
| ra | double | deg | J2000 right ascension (r') | |||
| dec | double | deg | J2000 declination (r') | |||
| cx | double | unit vector for ra+dec | ||||
| cy | double | unit vector for ra+dec | ||||
| cz | double | unit vector for ra+dec | ||||
| primTarget | int | Bit mask of primary target categories the object was selected in. | ||||
| secTarget | int | Bit mask of secondary target categories the object was selected in. | ||||
| extinction_u | float | mag | Extinction in each filter | |||
| extinction_g | float | mag | Extinction in each filter | |||
| extinction_r | float | mag | Extinction in each filter | |||
| extinction_i | float | mag | Extinction in each filter | |||
| extinction_z | float | mag | Extinction in each filter | |||
| htmID | long | 20-deep hierarchical trangular mesh ID of this object | ||||
| fieldID | long | Link to the field this object is in | ||||
| specObjID | long | Pointer to the spectrum of object, if exists, else 0 | ||||
| size | float | computed: =SQRT(mRrCc_r/2.0) |
Contains the spatial cross-match between DR8 primaries and DR7 primaries
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| dr7objID | long | Unique DR7 identifier composed from [skyVersion,rerun,run,camcol,field,obj]. | ||||
| dr8objID | long | Unique DR8 identifier composed from [skyVersion,rerun,run,camcol,field,obj]. | ||||
| distance | double | Distance in arcmin between the DR7 and DR8 positions | ||||
| skyVersion | int | 0 = OPDB target, 1 = OPDB best | ||||
| run | int | Run number | ||||
| rerun | int | Rerun number | ||||
| camcol | int | Camera column | ||||
| field | int | Field number | ||||
| obj | int | The object id within a field. Usually changes between reruns of the same field. | ||||
| nChild | int | Number of children if this is a composite object that has been deblended. BRIGHT (in a flags sense) objects also have nchild == 1, the non-BRIGHT sibling. | ||||
| type | int | Morphological type classification of the object. | ||||
| probPSF | float | Probability that the object is a star. Currently 0 if type == 3 (galaxy), 1 if type == 6 (star). | ||||
| insideMask | int | Flag to indicate whether object is inside a mask and why | ||||
| flags | long | Photo Object Attribute Flags | ||||
| psfMag_u | float | mag | PSF flux | |||
| psfMag_g | float | mag | PSF flux | |||
| psfMag_r | float | mag | PSF flux | |||
| psfMag_i | float | mag | PSF flux | |||
| psfMag_z | float | mag | PSF flux | |||
| psfMagErr_u | float | mag | PSF flux error | |||
| psfMagErr_g | float | mag | PSF flux error | |||
| psfMagErr_r | float | mag | PSF flux error | |||
| psfMagErr_i | float | mag | PSF flux error | |||
| psfMagErr_z | float | mag | PSF flux error | |||
| petroMag_u | float | mag | Petrosian flux | |||
| petroMag_g | float | mag | Petrosian flux | |||
| petroMag_r | float | mag | Petrosian flux | |||
| petroMag_i | float | mag | Petrosian flux | |||
| petroMag_z | float | mag | Petrosian flux | |||
| petroMagErr_u | float | mag | Petrosian flux error | |||
| petroMagErr_g | float | mag | Petrosian flux error | |||
| petroMagErr_r | float | mag | Petrosian flux error | |||
| petroMagErr_i | float | mag | Petrosian flux error | |||
| petroMagErr_z | float | mag | Petrosian flux error | |||
| petroR50_r | float | arcsec | Radius containing 50% of Petrosian flux | |||
| petroR90_r | float | arcsec | Radius containing 90% of Petrosian flux | |||
| modelMag_u | float | mag | better of DeV/Exp magnitude fit | |||
| modelMag_g | float | mag | better of DeV/Exp magnitude fit | |||
| modelMag_r | float | mag | better of DeV/Exp magnitude fit | |||
| modelMag_i | float | mag | better of DeV/Exp magnitude fit | |||
| modelMag_z | float | mag | better of DeV/Exp magnitude fit | |||
| modelMagErr_u | float | mag | better of DeV/Exp magnitude fit error | |||
| modelMagErr_g | float | mag | better of DeV/Exp magnitude fit error | |||
| modelMagErr_r | float | mag | better of DeV/Exp magnitude fit error | |||
| modelMagErr_i | float | mag | better of DeV/Exp magnitude fit error | |||
| modelMagErr_z | float | mag | better of DeV/Exp magnitude fit error | |||
| mRrCc_r | float | Adaptive (<r^2> + <c^2>) | ||||
| mRrCcErr_r | float | Error in adaptive (<r^2> + <c^2>) | ||||
| lnLStar_r | float | Star ln(likelihood) | ||||
| lnLExp_r | float | Exponential disk fit ln(likelihood) | ||||
| lnLDeV_r | float | DeVaucouleurs fit ln(likelihood) | ||||
| status | int | Status of the object in the survey | ||||
| ra | double | deg | J2000 right ascension (r') | |||
| dec | double | deg | J2000 declination (r') | |||
| cx | double | unit vector for ra+dec | ||||
| cy | double | unit vector for ra+dec | ||||
| cz | double | unit vector for ra+dec | ||||
| primTarget | int | Bit mask of primary target categories the object was selected in. | ||||
| secTarget | int | Bit mask of secondary target categories the object was selected in. | ||||
| extinction_u | float | mag | Extinction in each filter | |||
| extinction_g | float | mag | Extinction in each filter | |||
| extinction_r | float | mag | Extinction in each filter | |||
| extinction_i | float | mag | Extinction in each filter | |||
| extinction_z | float | mag | Extinction in each filter | |||
| htmID | long | 20-deep hierarchical trangular mesh ID of this object | ||||
| fieldID | long | Link to the field this object is in | ||||
| specObjID | long | Pointer to the spectrum of object, if exists, else 0 | ||||
| size | float | computed: =SQRT(mRrCc_r/2.0) |
The annulus-averaged flux profiles of SDSS photo object
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| bin | int | bin number (0..14) | ||||
| band | int | u,g,r,i,z (0..4) | ||||
| profMean | float | nanomaggies/arcsec^2 | Mean flux in annulus | |||
| profErr | float | nanomaggies/arcsec^2 | Standard deviation of mean pixel flux in annulus | |||
| objID | long | links to the photometric object |
The photometrically estimated redshifts for all objects in the Galaxy view
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| objID | long | unique ID pointing to Galaxy table | ||||
| z | float | photometric redshift; estimated by robust fit to nearest neighbors in a reference set | ||||
| zErr | float | estimated error of the photometric redshift; if zErr=-1000, all the proceeding columns are invalid | ||||
| nnCount | int | nearest neighbors after excluding the outliers; maximal value is 100, much smaller value indicates poor estimate | ||||
| nnVol | float | gives the color space bounding volume of the nnCount nearest neighbors; large value indicates poor estimate | ||||
| nnIsInside | int | shows if the object to be estimated is inside of the k-nearest neighbor box; 0 indicates poor estimate | ||||
| nnObjID | long | objID of the (first) nearest neighbor | ||||
| nnSpecz | float | spectroscopic redshift of the (first) nearest neighbor | ||||
| nnFarObjID | long | objID of the farthest neighbor | ||||
| nnAvgZ | float | average redshift of the nearest neighbors; if singificantly different from z, this might be a better estimate than z | ||||
| distMod | float | the distance modulus for Omega=0.3, Lambda=0.7 cosmology | ||||
| lumDist | float | the luminosity distance for Omega=0.3, Lambda=0.7 cosmology | ||||
| chisq | float | the chi-square value for the best NNLS template fit | ||||
| rnorm | float | the residual norm value for the best NNLS template fit | ||||
| nTemplates | int | number of templates used in the fitting; if nTemplates=0 all the proceeding columns are invalid and may be filled with value -9999 | ||||
| synthU | float | synthetic u' magnitude calculated from the fitted templates | ||||
| synthG | float | synthetic g' magnitude calculated from the fitted templates | ||||
| synthR | float | synthetic r' magnitude calculated from the fitted templates | ||||
| synthI | float | synthetic i' magnitude calculated from the fitted templates | ||||
| synthZ | float | synthetic z' magnitude calculated from the fitted templates | ||||
| kcorrU | float | k correction for z=0 | ||||
| kcorrG | float | k correction for z=0 | ||||
| kcorrR | float | k correction for z=0 | ||||
| kcorrI | float | k correction for z=0 | ||||
| kcorrZ | float | k correction for z=0 | ||||
| kcorrU01 | float | k correction for z=0.1 | ||||
| kcorrG01 | float | k correction for z=0.1 | ||||
| kcorrR01 | float | k correction for z=0.1 | ||||
| kcorrI01 | float | k correction for z=0.1 | ||||
| kcorrZ01 | float | k correction for z=0.1 | ||||
| absMagU | float | rest frame u' abs magnitude | ||||
| absMagG | float | rest frame g' abs magnitude | ||||
| absMagR | float | rest frame r' abs magnitude | ||||
| absMagI | float | rest frame i' abs magnitude | ||||
| absMagZ | float | rest frame z' abs magnitude |
The photometrically estimated redshifts for all objects in the Galaxy view
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| objID | long | unique ID pointing to Galaxy table | ||||
| z | float | photometric redshift; estimated by the Random Forest method | ||||
| zErr | float | estimated error of the photometric redshift | ||||
| distMod | float | the distance modulus for Omega=0.3, Lambda=0.7 cosmology | ||||
| lumDist | float | the luminosity distance for Omega=0.3, Lambda=0.7 cosmology | ||||
| chisq | float | the chi-square value for the best NNLS template fit | ||||
| rnorm | float | the residual norm value for the best NNLS template fit | ||||
| nTemplates | int | number of templates used in the fitting; if nTemplates=0 all the proceeding columns are invalid and may be filled with value -9999 | ||||
| synthU | float | synthetic u' magnitude calculated from the fitted templates | ||||
| synthG | float | synthetic g' magnitude calculated from the fitted templates | ||||
| synthR | float | synthetic r' magnitude calculated from the fitted templates | ||||
| synthI | float | synthetic i' magnitude calculated from the fitted templates | ||||
| synthZ | float | synthetic z' magnitude calculated from the fitted templates | ||||
| kcorrU | float | k correction for z=0 | ||||
| kcorrG | float | k correction for z=0 | ||||
| kcorrR | float | k correction for z=0 | ||||
| kcorrI | float | k correction for z=0 | ||||
| kcorrZ | float | k correction for z=0 | ||||
| kcorrU01 | float | k correction for z=0.1 | ||||
| kcorrG01 | float | k correction for z=0.1 | ||||
| kcorrR01 | float | k correction for z=0.1 | ||||
| kcorrI01 | float | k correction for z=0.1 | ||||
| kcorrZ01 | float | k correction for z=0.1 | ||||
| absMagU | float | rest frame u' abs magnitude | ||||
| absMagG | float | rest frame g' abs magnitude | ||||
| absMagR | float | rest frame r' abs magnitude | ||||
| absMagI | float | rest frame i' abs magnitude | ||||
| absMagZ | float | rest frame z' abs magnitude |
Template coefficients for the PhotozRF table.
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| objID | long | unique ID pointing to Galaxy table | ||||
| templateID | int | id for the spectral template | ||||
| coeff | float | coefficient of the template |
Template coefficients for the Photoz table.
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| objID | long | unique ID pointing to Galaxy table | ||||
| templateID | int | id for the spectral template | ||||
| coeff | float | coefficient of the template |
Which objects are in the coverage area of which plates
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| plate2targetid | int | primary key | ||||
| plate | int | plate number | ||||
| plateid | long | plate identification number in plateX | ||||
| objid | long | object identification number in sppTargets | ||||
| loadVersion | int | Load Version |
Contains data from a given plate used for spectroscopic observations
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| plateID | long | Unique ID, composite of plate number and MJD | ||||
| firstRelease | string | Name of release that this plate/mjd/rerun was first distributed in | ||||
| plate | int | Plate number | ||||
| mjd | int | days | MJD of observation (last) | |||
| mjdList | string | List of contributing MJDs [from spPlate header] | ||||
| survey | string | Name of survey [from platelist product] | ||||
| programName | string | Name of program [from platelist product] | ||||
| instrument | string | Instrument used (SDSS or BOSS spectrograph) | ||||
| chunk | string | Name of tiling chunk [from platelist product] | ||||
| plateRun | string | Drilling run for plate [from platelist product] | ||||
| designComments | string | Comments on the plate design from plate plans [from platelist product] | ||||
| plateQuality | string | Characterization of plate quality | ||||
| qualityComments | string | Comments on reason for plate quality | ||||
| plateSN2 | float | Overall signal to noise measure for plate (only set for SDSS plates) | ||||
| deredSN2 | float | Dereddened overall signal to noise measure for plate (only set for BOSS plates) | ||||
| ra | double | deg | RA, J2000 [from spPlate header] | |||
| dec | double | deg | Dec, J2000 [from spPlate header] | |||
| run2d | string | 2D reduction rerun of plate | ||||
| run1d | string | 1D reduction rerun of plate | ||||
| runsspp | string | SSPP reduction rerun of plate ("none" if not run) | ||||
| tile | int | Tile number for SDSS-I, -II plates (-1 for SDSS-III) [from platelist product] | ||||
| designID | int | Design number number for SDSS-III plates (-1 for SDSS-I, -II) [from platelist product] | ||||
| locationID | int | Location number number for SDSS-III plates (-1 for SDSS-I, -II) [from platelist product] | ||||
| iopVersion | string | IOP Version [from spPlate header] | ||||
| camVersion | string | Camera code version [from spPlate header] | ||||
| taiHMS | string | Time in string format [from spPlate header] | ||||
| dateObs | string | Date of 1st row [from spPlate header] | ||||
| timeSys | string | Time System [from spPlate header] | ||||
| cx | double | x of Normal unit vector in J2000 | ||||
| cy | double | y of Normal unit vector in J2000 | ||||
| cz | double | z of Normal unit vector in J2000 | ||||
| cartridgeID | int | ID of cartridge used for the observation [from spPlate header] | ||||
| tai | double | sec | Mean time (TAI) [from spPlate header] | |||
| taiBegin | double | sec | Beginning time (TAI) [from spPlate header] | |||
| taiEnd | double | sec | Ending time (TAI) [from spPlate header] | |||
| airmass | float | Airmass at central TAI time [from spPlate header] | ||||
| mapMjd | int | days | Map MJD [from spPlate header] | |||
| mapName | string | ID of mapping file [from spPlate header] | ||||
| plugFile | string | Full name of mapping file [from spPlate header] | ||||
| expTime | float | sec | Total Exposure time [from spPlate header] | |||
| expTimeB1 | float | sec | exposure time in B1 spectrograph [from spPlate header] | |||
| expTimeB2 | float | sec | exposure time in B2 spectrograph [from spPlate header] | |||
| expTimeR1 | float | sec | exposure time in R1 spectrograph [from spPlate header] | |||
| expTimeR2 | float | sec | exposure time in R2 spectrograph [from spPlate header] | |||
| vers2d | string | idlspec2d version used during 2d reduction [from spPlate header] | ||||
| verscomb | string | idlspec2d version used during combination of multiple exposures [from spPlate header] | ||||
| vers1d | string | idlspec2d version used during redshift fitting [from spPlate header] | ||||
| snturnoff | float | Signal to noise measure for MS turnoff stars on plate (-9999 if not appropriate) | ||||
| nturnoff | float | Number of MS turnoff stars on plate | ||||
| nExp | int | Number of exposures total [from spPlate header] | ||||
| nExpB1 | int | Number of exposures in B1 spectrograph [from spPlate header] | ||||
| nExpB2 | int | Number of exposures in B2 spectrograph [from spPlate header] | ||||
| nExpR1 | int | Number of exposures in R1 spectrograph [from spPlate header] | ||||
| nExpR2 | int | Number of exposures in R2 spectrograph [from spPlate header] | ||||
| sn1_g | float | (S/N)^2 at g=20.20 for spectrograph #1 [from spPlate header] | ||||
| sn1_r | float | (S/N)^2 at r=20.25 for spectrograph #1 [from spPlate header] | ||||
| sn1_i | float | (S/N)^2 at i=19.90 for spectrograph #1 [from spPlate header] | ||||
| sn2_g | float | (S/N)^2 at g=20.20 for spectrograph #2 [from spPlate header] | ||||
| sn2_r | float | (S/N)^2 at r=20.25 for spectrograph #2 [from spPlate header] | ||||
| sn2_i | float | (S/N)^2 at i=19.90 for spectrograph #2 [from spPlate header] | ||||
| dered_sn1_g | float | Dereddened (S/N)^2 at g=20.20 for spectrograph #1 [from spPlate header] | ||||
| dered_sn1_r | float | Dereddened (S/N)^2 at r=20.25 for spectrograph #1 [from spPlate header] | ||||
| dered_sn1_i | float | Dereddened (S/N)^2 at i=19.90 for spectrograph #1 [from spPlate header] | ||||
| dered_sn2_g | float | Dereddened (S/N)^2 at g=20.20 for spectrograph #2 [from spPlate header] | ||||
| dered_sn2_r | float | Dereddened (S/N)^2 at r=20.25 for spectrograph #2 [from spPlate header] | ||||
| dered_sn2_i | float | Dereddened (S/N)^2 at i=19.90 for spectrograph #2 [from spPlate header] | ||||
| helioRV | float | km/s | Heliocentric velocity correction [from spPlate header] | |||
| gOffStd | float | mag | Mean g-band mag difference (spectro - photo) for standards [from spPlate header] | |||
| gRMSStd | float | mag | Standard deviation of g-band mag difference (spectro - photo) for standards [from spPlate header] | |||
| rOffStd | float | mag | Mean r-band mag difference (spectro - photo) for standards [from spPlate header] | |||
| rRMSStd | float | mag | Standard deviation of r-band mag difference (spectro - photo) for standards [from spPlate header] | |||
| iOffStd | float | mag | Mean i-band mag difference (spectro - photo) for standards [from spPlate header] | |||
| iRMSStd | float | mag | Standard deviation of i-band mag difference (spectro - photo) for standards [from spPlate header] | |||
| grOffStd | float | mag | Mean g-band mag difference (spectro - photo) for standards [from spPlate header] | |||
| grRMSStd | float | mag | Standard deviation of g-band mag difference (spectro - photo) for standards [from spPlate header] | |||
| riOffStd | float | mag | Mean r-band mag difference (spectro - photo) for standards [from spPlate header] | |||
| riRMSStd | float | mag | Standard deviation of r-band mag difference (spectro - photo) for standards [from spPlate header] | |||
| gOffGal | float | mag | Mean g-band mag difference (spectro - photo) for galaxies [from spPlate header] | |||
| gRMSGal | float | mag | Standard deviation of g-band mag difference (spectro - photo) for galaxies [from spPlate header] | |||
| rOffGal | float | mag | Mean r-band mag difference (spectro - photo) for galaxies [from spPlate header] | |||
| rRMSGal | float | mag | Standard deviation of r-band mag difference (spectro - photo) for galaxies [from spPlate header] | |||
| iOffGal | float | mag | Mean i-band mag difference (spectro - photo) for galaxies [from spPlate header] | |||
| iRMSGal | float | mag | Standard deviation of i-band mag difference (spectro - photo) for galaxies [from spPlate header] | |||
| grOffGal | float | mag | Mean g-band mag difference (spectro - photo) for galaxies [from spPlate header] | |||
| grRMSGal | float | mag | Standard deviation of g-band mag difference (spectro - photo) for galaxies [from spPlate header] | |||
| riOffGal | float | mag | Mean r-band mag difference (spectro - photo) for galaxies [from spPlate header] | |||
| riRMSGal | float | mag | Standard deviation of r-band mag difference (spectro - photo) for galaxies [from spPlate header] | |||
| nGuide | int | Number of guider camera frames taken during the exposure [from spPlate header] | ||||
| seeing20 | float | 20th-percentile of seeing during exposure (arcsec) [from spPlate header] | ||||
| seeing50 | float | 50th-percentile of seeing during exposure (arcsec) [from spPlate header] | ||||
| seeing80 | float | 80th-percentile of seeing during exposure (arcsec) [from spPlate header] | ||||
| rmsoff20 | float | 20th-percentile of RMS offset of guide fibers (arcsec) [from spPlate header] | ||||
| rmsoff50 | float | 50th-percentile of RMS offset of guide fibers (arcsec) [from spPlate header] | ||||
| rmsoff80 | float | 80th-percentile of RMS offset of guide fibers (arcsec) [from spPlate header] | ||||
| airtemp | float | deg Celsius | Air temperature in the dome [from spPlate header] | |||
| sfd_used | int | Were the SFD dust maps applied to the output spectrum? (0 = no, 1 = yes) | ||||
| xSigma | float | sigma of gaussian fit to spatial profile[from spPlate header] | ||||
| xSigMin | float | minimum of xSigma for all exposures [from spPlate header] | ||||
| xSigMax | float | maximum of xSigma for all exposures [from spPlate header] | ||||
| wSigma | float | sigma of gaussian fit to arc-line profiles in wavelength direction [from spPlate header] | ||||
| wSigMin | float | minimum of wSigma for all exposures [from spPlate header] | ||||
| wSigMax | float | maximum of wSigma for all exposures [from spPlate header] | ||||
| xChi2 | float | [from spPlate header] | ||||
| xChi2Min | float | [from spPlate header] | ||||
| xChi2Max | float | [from spPlate header] | ||||
| skyChi2 | float | average chi-squared from sky subtraction from all exposures [from spPlate header] | ||||
| skyChi2Min | float | minimum skyChi2 over all exposures [from spPlate header] | ||||
| skyChi2Max | float | maximum skyChi2 over all exposures [from spPlate header] | ||||
| fBadPix | float | Fraction of pixels that are bad (total) [from spPlate header] | ||||
| fBadPix1 | float | Fraction of pixels that are bad (spectrograph #1) [from spPlate header] | ||||
| fBadPix2 | float | Fraction of pixels that are bad (spectrograph #2) [from spPlate header] | ||||
| status2d | string | Status of 2D extraction | ||||
| statuscombine | string | Status of combination of multiple MJDs | ||||
| status1d | string | Status of 1D reductions | ||||
| nTotal | int | Number of objects total [calculated from spZbest file] | ||||
| nGalaxy | int | Number of objects classified as galaxy [calculated from spZbest file] | ||||
| nQSO | int | Number of objects classified as QSO [calculated from spZbest file] | ||||
| nStar | int | Number of objects classified as Star [calculated from spZbest file] | ||||
| nSky | int | Number of sky objects [calculated from spZbest file] | ||||
| nUnknown | int | Number of objects with zWarning set non-zero (such objects still classified as star, galaxy or QSO) [calculated from spZbest file] | ||||
| isBest | int | is this plateX entry the best observation of the plate | ||||
| isPrimary | int | is this plateX entry both good and the best observation of the plate | ||||
| isTile | int | is this plate the best representative of its tile (only set for "legacy" program plates) | ||||
| ha | float | deg | hour angle of design [from plPlugMapM file] | |||
| mjdDesign | int | MJD designed for [from plPlugMapM file] | ||||
| theta | float | cartridge position angle [from plPlugMapM file] | ||||
| fscanVersion | string | version of fiber scanning software [from plPlugMapM file] | ||||
| fmapVersion | string | version of fiber mapping software [from plPlugMapM file] | ||||
| fscanMode | string | 'slow', 'fast', or 'extreme' [from plPlugMapM file] | ||||
| fscanSpeed | int | speed of scan [from plPlugMapM file] | ||||
| htmID | long | 20 deep Hierarchical Triangular Mesh ID | ||||
| loadVersion | int | Load Version |
This table contains the radii for the Profiles tabl
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| bin | int | bin | ||||
| cell | int | the first cell in the annulus | ||||
| sinc | int | sinc shift (0:no, 1:yes) | ||||
| rInner | double | arcsec | Inner radius of the bin | |||
| rOuter | double | srcsec | Outer radius of the bin | |||
| aAnn | double | arcsec^2 | The area of the annulus | |||
| aDisk | double | arcsec^2 | The area of the disk to outerRadius |
Proper motions combining SDSS and recalibrated USNO-B astrometry
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| delta | float | arcsec | Distance between this object and the nearest matching USNO-B object. | |||
| match | int | Number of objects in USNO-B which matched this object within a 1 arcsec radius. If negative, then the nearest matching USNO-B object itself matched more than 1 SDSS object. | ||||
| pmL | float | mas/year | Proper motion in galactic longitude. | |||
| pmB | float | mas/year | Proper motion in galactic latitude. | |||
| pmRa | float | mas/year | Proper motion in right ascension. | |||
| pmDec | float | mas/year | Proper motion in declination. | |||
| pmRaErr | float | mas/year | Error in proper motion in right ascension. | |||
| pmDecErr | float | mas/year | Error in proper motion in declination. | |||
| sigRa | float | mas | RMS residual for the proper motion fit in r.a. | |||
| sigDec | float | mas | RMS residual for the proper motion fit in dec. | |||
| nFit | int | Number of detections used in the fit including the SDSS detection (thus, the number of plates the object was detected on in USNO-B plus one). | ||||
| O | float | mag | Recalibrated USNO-B O magnitude, recalibrated to SDSS g | |||
| E | float | mag | Recalibrated USNO-B E magnitude, recalibrated to SDSS r | |||
| J | float | mag | Recalibrated USNO-B J magnitude, recalibrated to SDSS g | |||
| F | float | mag | Recalibrated USNO-B F magnitude, recalibrated to SDSS r | |||
| N | float | mag | Recalibrated USNO-B N magnitude, recalibrated to SDSS i | |||
| dist20 | float | arcsec | Distance to the nearest neighbor with g < 20 | |||
| dist22 | float | arcsec | Distance to the nearest neighbor with g < 22 | |||
| objid | long | unique id, points to photoObj |
This table keeps the record of publishing into a tabl
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| name | string | the name of the table we publish into | ||||
| nrows | long | the number of rows published | ||||
| tend | dateTime | the time the table was published | ||||
| loadversion | int | the taskid where it came from |
Store the results of performance tests her
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| query | string | query name | ||||
| cpu_sec | double | sec | CPU time | |||
| elapsed_time | double | sec | elapsed time | |||
| physical_IO | double | Physical IO | ||||
| row_count | long | row count | ||||
| time | dateTime | timestamp | ||||
| comment | string | comment describing test paraeters |
RC3 information for matches to SDSS photometr
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| objID | long | Unique SDSS identifier composed from [skyVersion,rerun,run,camcol,field,obj]. | ||||
| RA | double | deg -/D J2000 right ascension in RC3 | ||||
| DEC | double | deg -/D J2000 declination in RC3 | ||||
| NAME1 | string | designation #1 (Names or NGC and IC) | ||||
| NAME2 | string | designation #2 (UGC, ESO, MCG, UGCA, CGCG) | ||||
| NAME3 | string | designation #3 (other) | ||||
| PGC | string | Principal Galaxy Catalog number (Paturel et al. 1989) | ||||
| HUBBLE | string | revised Hubble type, coded as in RC2 (Section 3.3.a, page 13). | ||||
| LOGD_25 | float | mean decimal logarithm of the apparent major isophotal diameter measured at or reduced to surface brightness level mu_B = 25.0 B-mag/arcsec^2, as explained in Section 3.4.a, page 21. Unit of D is 0.1 arcmin to avoid negative entries. | ||||
| LOGD_25Q | string | quality flag for isophotal diameter ("?" if bad) | ||||
| LOGD_25ERR | float | error on mean decimal logarithm of the apparent major isophotal diameter | ||||
| PA | float | deg | position angle (east of north) | |||
| BT | float | mag | total (asymptotic) magnitude in the B system | |||
| BT_S | string | source code for BT | ||||
| BTQ | string | quality flag total magnitude ("?" if bad) | ||||
| BTERR | float | mag | error in total (asymptotic) magnitude in the B system | |||
| BMVT | float | mag | total (asymptotic) color index in Johnson B-V | |||
| BMVTQ | string | quality flag ("?" if bad) | ||||
| BMVTERR | float | mag | error in total (asymptotic) color index in Johnson B-V | |||
| BMVE | float | mag | color index within effective aperture in Johnson B-V | |||
| BMVEQ | string | quality flag ("?" if bad) | ||||
| BMVEERR | float | mag | error in color index within effective aperture in Johnson B-V | |||
| M21 | float | 21-cm emission line magnitude, defined by by m_21 = 21.6 - 2.5 log(S_H), where S_H is the measured neutral hydrogen flux density in units of 10^-24 W/m^2. | ||||
| M21Q | string | quality flag ("?" if bad) | ||||
| M21ERR | float | error in 21-cm emission line magnitude | ||||
| V21 | float | km/s | mean heliocentric radial velocity from HI observations | |||
| V21Q | string | quality flag ("?" if bad) | ||||
| V21ERR | float | km/s | error in heliocentric radial velocity | |||
| HUBBLE_SRC | string | sources of revised type estimate | ||||
| N_L | int | number of luminosity class estimates | ||||
| LOGR_25 | float | mean decimal logarithm of the ratio of the major isophotal diameter, D_25, to the minor isophotal diameter, d_25, measured at or reduced to the surface brightness level mu_B = 25.0 B-mag/arcsec^2. | ||||
| LOGR_25Q | string | quality flag ("?" if bad) | ||||
| LOGR_25ERR | float | error in decimal logarithm of the ratio of the major isophotal diameter to minor | ||||
| AGB | float | mag | Burstein-Heiles Galactic extinction in B | |||
| MB | float | mag | photographic magnitude reduced to B_T system | |||
| MBQ | string | mag | quality flag ("?" if bad) | |||
| MBERR | float | mag | error in photograph magnitude | |||
| UMBT | float | mag | total (asymptotic) color index in Johnson U-B | |||
| UMBTQ | string | quality flag ("?" if bad) | ||||
| UMBTERR | float | mag | error in total (asymptotic) color index in Johnson U-B | |||
| UMBE | float | mag | color index within effective aperture in Johnson U-B | |||
| UMBEQ | string | quality flag ("?" if bad), | ||||
| UMBEERR | float | mag | error in color index within effective aperture in Johnson U-B | |||
| W20 | float | km/s | neutral hydrogen line full width (in km/s) measured at the 20% level (I_20/I_max) | |||
| W20Q | string | quality flag ("?" if bad) | ||||
| W20ERR | float | km/s | error in W20 | |||
| VOPT | float | km/s | mean heliocentric radial velocity from optical observations | |||
| VOPTQ | string | quality flag ("?" if bad) | ||||
| VOPTERR | float | km/s | error in mean heliocentric radial velocity from optical observations | |||
| SGL | double | deg | supergalactic longitude | |||
| SGB | double | deg | supergalactic latitude | |||
| TYPE | float | T = mean numerical index of stage along the Hubble sequence in the RC2 system (coded as explained in Section 3.3.c, page 16) | ||||
| TYPEQ | string | quality flag ("?" if bad) | ||||
| TYPEERR | float | error in T-type | ||||
| LOGA_E | float | decimal logarithm of the apparent diameter (in 0.1 arcmin) of the ``effective aperture,'' the circle centered on the nucleus within which one-half of the total B-band flux is emitted | ||||
| LOGA_EQ | string | quality flag ("?" if bad) | ||||
| LOGA_EERR | float | error in decimal logarithm of the apparent diameter (in 0.1 arcmin) of the ``effective aperture,'' | ||||
| AIB | float | mag | internal extinction (for correction to face-on), calcauled from size and T-type | |||
| MFIR | float | far-infrared magnitude calculated from m_FIR = - 20.0 - 2.5 logFIR, where FIR is the far infrared continuum flux measured at 60 and 100 microns as listed in the IRAS Point Source Catalog (1987). | ||||
| BMVT0 | float | mag | total B-V color index corrected for Galactic and internal extinction, and for redshift | |||
| MPE | float | mag/sq arcmin | mean B-band surface brightness in magnitudes per square arcmin (B-mag/arcmin^2) within the effective aperture A_e, and its mean error, as given by the relation MPE = B_T + 0.75 + 5logA_e - 5.26. | |||
| MPEQ | string | quality flag ("?" if bad) | ||||
| MPEERR | float | mag/sq arcmin | error in mean B-band surface brightness | |||
| W50 | float | km/s | neutral hydrogen line full width (in km/s) measured at the 50% level (I_20/I_max) | |||
| W50Q | string | quality flag ("?" if bad) | ||||
| W50ERR | float | km/s | error in neutral hydrogen line full width (in km/s) measured at the 50% level (I_20/I_max) | |||
| VGSR | float | km/s | the weighted mean of the neutral hydrogen and optical velocities, corrected to the ``Galactic standard of rest'' | |||
| L | float | |||||
| LQ | string | quality flag ("?" if bad) | ||||
| LERR | float | mean numerical luminosity class in the RC2 system | ||||
| LOGD0 | float | decimal logarithm of the isophotal major diameter corrected to ``face-on'' (inclination = 0 degrees), and corrected for Galactic extinction to A_g = 0, but not for redshift | ||||
| SA21 | float | mag | HI line self-absorption in magnitudes (for correction to face-on), calculated from logR and T >= 1 | |||
| BT0 | float | mag | B_T^0 = total ``face-on'' magnitude corrected for Galactic and internal extinction, and for redshift | |||
| UMBT0 | float | mag | (U-B)_T^0 = total U-B color index corrected for Galactic and internal extinction, and for redshift | |||
| MP25 | float | mag/sq arcmin | the mean surface brightness in magnitudes per square arcmin (B-mag/arcmin^2) within the mu_B = 25.0 B-mag/arcsec^2 elliptical isophote of major axis D_25 and axis ratio R_25 | |||
| MP25Q | string | quality flag ("?" if bad) | ||||
| MP25ERR | float | mag/sq arcmin | error inthe mean surface brightness within the mu_B = 25.0 B-mag/arcsec^2 | |||
| HI | float | corrected neutral hydrogen index, which is the difference m_21^0 - B_T^0 between the corrected (face-on) 21-cm emission line magnitude and the similarly corrected magnitude in the B_T system. | ||||
| V3K | float | km/s | the weighted mean velocity corrected to the reference frame defined by the 3 K microwave background radiation |
ROSAT All-Sky Survey information for matches to SDSS photometr
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| OBJID | long | Unique SDSS identifier composed from [skyVersion,rerun,run,camcol,field,obj]. | ||||
| SOURCENAME | string | name of source in ROSAT | ||||
| RA | double | deg | J2000 right ascension of ROSAT source | |||
| DEC | double | deg | J2000 declination of ROSAT source | |||
| RADECERR | float | arcsec | error in coordinates | |||
| FLAGS | string | screening flags (see ROSAT documentation) | ||||
| FLAGS2 | string | screening flags (see ROSAT documentation) | ||||
| CPS | float | counts per second in broad band | ||||
| CPS_ERR | float | error in count rate | ||||
| BGCPS | float | counts per second from background | ||||
| EXPTIME | float | sec | exposure time | |||
| HR1 | float | hardness ratio 1 | ||||
| HR1_ERR | float | error in hardness ratio 1 | ||||
| HR2 | float | hardness ratio 2 | ||||
| HR2_ERR | float | error in hardness ratio 2 | ||||
| EXT | float | arcsec | source extent | |||
| EXTL | float | likelihood of source extent | ||||
| SRCL | float | likelihood of source detection | ||||
| EXTR | float | arcsec | extraction radius | |||
| PRIORITY | string | priority flags (Sliding window detection history using either the background map (M) or the local background (B); 0 = no detection, 1 = detection; order of flags: M-broad, L-broad, M-hard, L-hard, M-soft, L-soft | ||||
| ERANGE | string | pulse height amplitude range with highest detection likelihood; A: 11-41, B: 52-201, C: 52-90, D: 91-201 ' ' or 'b' means 'broad' (11-235) | ||||
| VIGF | float | vignetting factor | ||||
| ORGDAT | string | date when source was included (format: yymmdd; 000000: removed) | ||||
| MODDAT | string | date when source was modified (format: yymmdd; 000000: removed) | ||||
| ID | int | number of identification candidates in correlation catalog | ||||
| FIELDID | int | identification number of SASS field | ||||
| SRCNUM | int | SASS source number in SASS field | ||||
| RCT1 | int | number of nearby RASS detections with distances between 0 and 5 arcmin | ||||
| RCT2 | int | number of nearby RASS detections with distances between 5 and 10 arcmin | ||||
| RCT3 | int | number of nearby RASS detections with distances between 10 and 15 arcmin | ||||
| ITB | string | start time of observation (yymmdd.ff) | ||||
| ITE | string | end time of observation (yymmdd.ff) | ||||
| RL | int | reliability of source detection (0 to 99, with 99 being highest) | ||||
| CAT | string | which catalog the source is in (faint or bright) |
Record the ipAddr and timestamps of the last n querie
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| ipAddr | string | |||||
| lastQueryTime | dateTime |
Definition of the different region
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| regionid | long | |||||
| id | long | key of the region pointing into other tables | ||||
| type | string | type of the region (STRIPE|STAVE|...) | ||||
| comment | string | description of the region | ||||
| ismask | int | 0: region, 1: to be excluded | ||||
| area | double | deg^2 | area of region | |||
| regionString | string | the string representation of the region | ||||
| regionBinary | int | the precompiled XML description of region |
Tracks the parentage which regions contribute to which boxe
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| regionType | string | type of parent, (TIGEOM) | ||||
| id | long | the object id of the other parent region | ||||
| boxType | string | type of child (TILEBOX, SKYBOX) | ||||
| boxid | long | regionid of child |
Contains the arcs of a Region with their endpoint
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| arcid | int | unique id of the arc | ||||
| regionid | long | unique region identifier | ||||
| convexid | long | convex identifier | ||||
| patch | int | id of the patch | ||||
| state | int | state (3: bounding circle, 2:root, 1: hole) | ||||
| draw | int | 0:hide, 1: draw | ||||
| ra1 | double | ra of starting point of arc | ||||
| dec1 | double | dec of starting point of arc | ||||
| ra2 | double | ra of end point of arc | ||||
| dec2 | double | dec of end point of arc | ||||
| x | double | x of constraint normal vector | ||||
| y | double | y of constraint normal vector | ||||
| z | double | z of constraint normal vector | ||||
| c | double | offset of constraint | ||||
| length | double | deg | length of arc in degrees |
Defines the attributes of the patches of a given regio
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| regionid | long | Unique Region ID | ||||
| convexid | long | Unique Convex ID | ||||
| patchid | int | Unique patch number | ||||
| type | string | CAMCOL, RUN, STAVE, TILE, TILEBOX, SKYBOX, WEDGE, SECTOR... | ||||
| radius | double | arcmin | radius of bounding circle centered at ra, dec | |||
| ra | double | deg | right ascension of observation | |||
| dec | double | deg | declination of observation | |||
| x | double | x of centerpoint Normal unit vector in J2000 | ||||
| y | double | y of centerpoint Normal unit vector in J2000 | ||||
| z | double | z of centerpoint Normal unit vector in J2000 | ||||
| c | double | offset of the equation of plane | ||||
| htmid | long | 20 deep Hierarchical Triangular Mesh ID of centerpoint | ||||
| area | double | deg^2 | area of the patch | |||
| convexString | string | {x,y,z,c}+ representation of the convex of the patch |
Contains various rotation matrices between spherical coordinate system
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| mode | string | |||||
| row | int | |||||
| x | double | |||||
| y | double | |||||
| z | double |
Contains the basic parameters associated with a ru
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| skyVersion | int | 0 = OPDB target, 1 = OPDB best XXX | ||||
| run | int | Run number | ||||
| rerun | int | Rerun number | ||||
| mjd | int | days | MJD of observation | |||
| datestring | string | Human-readable date of observation | ||||
| stripe | int | Stripe number | ||||
| strip | string | Strip (N or S) | ||||
| xBore | double | deg | boresight offset perpendicular to great circle | |||
| fieldRef | int | Starting field number of full run (what MU_REF, MJD_REF refer to) | ||||
| lastField | int | last field of full run | ||||
| flavor | string | type of drift scan (from apacheraw, bias, calibration, engineering, ignore, and science) | ||||
| xBin | int | pix | binning amount perpendicular to scan direction | |||
| yBin | int | pix | binning amount in scan direction | |||
| nRow | int | pix | number of rows in output idR | |||
| mjdRef | double | days | MJD at row 0 of reference frame | |||
| muRef | double | deg | mu value at row 0 of reference field | |||
| lineStart | int | microsec | linestart rate betweeen each (binned) row | |||
| tracking | double | arcsec/sec | tracking rate | |||
| node | double | node of great circle, that is, its RA on the J2000 equator | ||||
| incl | double | inclination of great circle relative to J2000 equator | ||||
| comments | string | comments on the run | ||||
| qterm | float | arcsec/hr^2 | quadratic term in coarse astrometric solution | |||
| maxMuResid | float | arcsec | maximum residual from great circle in scan direction | |||
| maxNuResid | float | arcsec | maximum residual from great circle perpendicular to scan direction | |||
| startField | int | starting field for reduced data | ||||
| endField | int | ending field for reduced data | ||||
| photoVersion | string | photo version used | ||||
| dervishVersion | string | dervish version used | ||||
| astromVersion | string | astrom version used | ||||
| sasVersion | string | version of SAS used to produce CSV for this run |
The table contains values of the various manual nu shifts for run
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| run | int | Run id | ||||
| shift | double | deg | The nu shift applied |
This table contains most relevant survey constants and their physical unit
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| name | string | Name of the constant | ||||
| value | double | The numerical value in float | ||||
| unit | string | Its physical unit | ||||
| description | string | Short description |
Table holding site specific constant
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| name | string | Name | ||||
| value | string | Value | ||||
| comment | string | Description |
Table containing the list of DBs at this CAS site
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| dbname | string | Name of the database | ||||
| description | string | Short one-line description | ||||
| active | string | Is it active/visible? |
This table stores the full diagnostic snapshot after the last revisio
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| name | string | Name of object | ||||
| type | string | System type of the object (U:table, V:view, F: function, P: stored proc) | ||||
| count | long | Optional row count, where applicable |
Contains the spatial cross-match between DR8 SpecObjAll and DR7 primaries
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| specObjID | long | Unique DR8 ID based on PLATE, MJD, FIBERID, RUN2D | ||||
| dr7ObjID | long | Unique DR7 PhotoPrimary ID composed from [skyVersion,rerun,run,camcol,field,obj]. | ||||
| ra | double | deg | J2000 right ascension (r') | |||
| dec | double | deg | J2000 declination (r') | |||
| cx | double | unit vector for ra+dec | ||||
| cy | double | unit vector for ra+dec | ||||
| cz | double | unit vector for ra+dec | ||||
| skyVersion | int | 0 = OPDB target, 1 = OPDB best | ||||
| run | int | Run number | ||||
| rerun | int | Rerun number | ||||
| camcol | int | Camera column | ||||
| field | int | Field number | ||||
| obj | int | The object id within a field. Usually changes between reruns of the same field. | ||||
| nChild | int | Number of children if this is a composite object that has been deblended. BRIGHT (in a flags sense) objects also have nchild == 1, the non-BRIGHT sibling. | ||||
| type | int | Morphological type classification of the object. | ||||
| probPSF | float | Probability that the object is a star. Currently 0 if type == 3 (galaxy), 1 if type == 6 (star). | ||||
| insideMask | int | Flag to indicate whether object is inside a mask and why | ||||
| flags | long | Photo Object Attribute Flags | ||||
| psfMag_u | float | mag | PSF flux | |||
| psfMag_g | float | mag | PSF flux | |||
| psfMag_r | float | mag | PSF flux | |||
| psfMag_i | float | mag | PSF flux | |||
| psfMag_z | float | mag | PSF flux | |||
| psfMagErr_u | float | mag | PSF flux error | |||
| psfMagErr_g | float | mag | PSF flux error | |||
| psfMagErr_r | float | mag | PSF flux error | |||
| psfMagErr_i | float | mag | PSF flux error | |||
| psfMagErr_z | float | mag | PSF flux error | |||
| petroMag_u | float | mag | Petrosian flux | |||
| petroMag_g | float | mag | Petrosian flux | |||
| petroMag_r | float | mag | Petrosian flux | |||
| petroMag_i | float | mag | Petrosian flux | |||
| petroMag_z | float | mag | Petrosian flux | |||
| petroMagErr_u | float | mag | Petrosian flux error | |||
| petroMagErr_g | float | mag | Petrosian flux error | |||
| petroMagErr_r | float | mag | Petrosian flux error | |||
| petroMagErr_i | float | mag | Petrosian flux error | |||
| petroMagErr_z | float | mag | Petrosian flux error | |||
| petroR50_r | float | arcsec | Radius containing 50% of Petrosian flux | |||
| petroR90_r | float | arcsec | Radius containing 90% of Petrosian flux | |||
| modelMag_u | float | mag | better of DeV/Exp magnitude fit | |||
| modelMag_g | float | mag | better of DeV/Exp magnitude fit | |||
| modelMag_r | float | mag | better of DeV/Exp magnitude fit | |||
| modelMag_i | float | mag | better of DeV/Exp magnitude fit | |||
| modelMag_z | float | mag | better of DeV/Exp magnitude fit | |||
| modelMagErr_u | float | mag | better of DeV/Exp magnitude fit error | |||
| modelMagErr_g | float | mag | better of DeV/Exp magnitude fit error | |||
| modelMagErr_r | float | mag | better of DeV/Exp magnitude fit error | |||
| modelMagErr_i | float | mag | better of DeV/Exp magnitude fit error | |||
| modelMagErr_z | float | mag | better of DeV/Exp magnitude fit error | |||
| mRrCc_r | float | Adaptive (<r^2> + <c^2>) | ||||
| mRrCcErr_r | float | Error in adaptive (<r^2> + <c^2>) | ||||
| lnLStar_r | float | Star ln(likelihood) | ||||
| lnLExp_r | float | Exponential disk fit ln(likelihood) | ||||
| lnLDeV_r | float | DeVaucouleurs fit ln(likelihood) | ||||
| status | int | Status of the object in the survey | ||||
| primTarget | int | Bit mask of primary target categories the object was selected in. | ||||
| secTarget | int | Bit mask of secondary target categories the object was selected in. | ||||
| extinction_u | float | mag | Extinction in each filter | |||
| extinction_g | float | mag | Extinction in each filter | |||
| extinction_r | float | mag | Extinction in each filter | |||
| extinction_i | float | mag | Extinction in each filter | |||
| extinction_z | float | mag | Extinction in each filter | |||
| htmID | long | 20-deep hierarchical trangular mesh ID of this object | ||||
| fieldID | long | Link to the field this object is in | ||||
| size | float | computed: =SQRT(mRrCc_r/2.0) | ||||
| pmRa | float | mas/year | Proper motion in right ascension. | |||
| pmDec | float | mas/year | Proper motion in declination. | |||
| pmL | float | mas/year | Proper motion in galactic longitude. | |||
| pmB | float | mas/year | Proper motion in galactic latitude. | |||
| pmRaErr | float | mas/year | Error in proper motion in right ascension. | |||
| pmDecErr | float | mas/year | Error in proper motion in declination. | |||
| delta | float | arcsec | Distance between this object and the nearest matching USNO-B object. | |||
| match | int | Number of objects in USNO-B which matched this object within a 1 arcsec radius. If negative, then the nearest matching USNO-B object itself matched more than 1 SDSS object. |
Contains the measured parameters for a spectrum
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| specObjID | long | Unique database ID based on PLATE, MJD, FIBERID, RUN2D | ||||
| bestObjID | long | Object ID of photoObj match (position-based) | ||||
| fluxObjID | long | Object ID of photoObj match (flux-based) | ||||
| targetObjID | long | Object ID of original target | ||||
| plateID | long | Database ID of Plate | ||||
| sciencePrimary | int | Best version of spectrum at this location (defines default view SpecObj) | ||||
| legacyPrimary | int | Best version of spectrum at this location, among Legacy plates | ||||
| seguePrimary | int | Best version of spectrum at this location, among SEGUE plates | ||||
| segue1Primary | int | Best version of spectrum at this location, among SEGUE-1 plates | ||||
| segue2Primary | int | Best version of spectrum at this location, among SEGUE-1 plates | ||||
| bossPrimary | int | Best version of spectrum at this location, among BOSS plates | ||||
| bossSpecObjID | int | Index of BOSS observation in spAll flat file | ||||
| firstRelease | string | Name of first release this object was associated with | ||||
| survey | string | Survey name | ||||
| instrument | string | Instrument used (SDSS or BOSS spectrograph) | ||||
| programname | string | Program name | ||||
| chunk | string | Chunk name | ||||
| platerun | string | Plate drill run name | ||||
| mjd | int | days | MJD of observation | |||
| plate | int | Plate number | ||||
| fiberID | int | Fiber ID | ||||
| run1d | string | 1D Reduction version of spectrum | ||||
| run2d | string | 2D Reduction version of spectrum | ||||
| tile | int | Tile number | ||||
| designID | int | Design ID number | ||||
| legacy_target1 | long | for Legacy program, target selection information at plate design | ||||
| legacy_target2 | long | for Legacy program target selection information at plate design, secondary/qa/calibration | ||||
| special_target1 | long | for Special program target selection information at plate design | ||||
| special_target2 | long | for Special program target selection information at plate design, secondary/qa/calibration | ||||
| segue1_target1 | long | SEGUE-1 target selection information at plate design, primary science selection | ||||
| segue1_target2 | long | SEGUE-1 target selection information at plate design, secondary/qa/calib selection | ||||
| segue2_target1 | long | SEGUE-2 target selection information at plate design, primary science selection | ||||
| segue2_target2 | long | SEGUE-2 target selection information at plate design, secondary/qa/calib selection | ||||
| boss_target1 | long | BOSS target selection information at plate | ||||
| ancillary_target1 | long | BOSS ancillary science target selection information at plate design | ||||
| ancillary_target2 | long | BOSS ancillary target selection information at plate design | ||||
| primTarget | long | target selection information at plate design, primary science selection (for backwards compatibility) | ||||
| secTarget | long | target selection information at plate design, secondary/qa/calib selection (for backwards compatibility) | ||||
| spectrographID | int | which spectrograph (1,2) | ||||
| sourceType | string | For Legacy, SEGUE-2 and BOSS science targets, type of object targeted as (target bits contain full information and are recommended) | ||||
| targetType | string | Nature of target: SCIENCE, STANDARD, or SKY | ||||
| ra | double | deg | DR8 Right ascension of fiber, J2000 | |||
| dec | double | deg | DR8 Declination of fiber, J2000 | |||
| cx | double | x of Normal unit vector in J2000 | ||||
| cy | double | y of Normal unit vector in J2000 | ||||
| cz | double | z of Normal unit vector in J2000 | ||||
| xFocal | float | mm | X focal plane position (+RA direction) | |||
| yFocal | float | mm | Y focal plane position (+Dec direction) | |||
| lambdaEff | float | Angstroms | Effective wavelength that hole was drilled for (accounting for atmopheric refraction) | |||
| blueFiber | int | Set to 1 if this hole was designated a "blue fiber", 0 if designated a "red fiber" (high redshift LRGs are preferentially in "red fibers") | ||||
| zOffset | float | microns | Washer thickness used (for backstopping BOSS quasar targets, so they are closer to 4000 Angstrom focal plan) | |||
| z | float | Final Redshift | ||||
| zErr | float | Redshift error | ||||
| zWarning | int | Bitmask of warning values; 0 means all is well | ||||
| class | string | Spectroscopic class (GALAXY, QSO, or STAR) | ||||
| subClass | string | Spectroscopic subclass | ||||
| rChi2 | float | Reduced chi-squared of best fit | ||||
| DOF | float | Degrees of freedom in best fit | ||||
| rChi2Diff | float | Difference in reduced chi-squared between best and second best fit | ||||
| z_noqso | float | Best redshift when excluding QSO fit (right redshift to use for galaxy targets) | ||||
| zErr_noqso | float | Error in "z_noqso" redshift | ||||
| zWarning_noqso | float | Warnings in "z_noqso" redshift | ||||
| class_noqso | string | Classification in "z_noqso" redshift | ||||
| subClass_noqso | string | Sub-classification in "z_noqso" redshift | ||||
| rChi2Diff_noqso | float | Reduced chi-squared difference from next best redshift, for "z_noqso" redshift | ||||
| z_person | float | Person-assigned redshift, if this object has been inspected | ||||
| class_person | string | Person-assigned classification, if this object has been inspected | ||||
| comments_person | string | Comments from person for inspected objects | ||||
| tFile | string | File name of best fit template source | ||||
| tColumn_0 | int | Which column of the template file corresponds to template #0 | ||||
| tColumn_1 | int | Which column of the template file corresponds to template #1 | ||||
| tColumn_2 | int | Which column of the template file corresponds to template #2 | ||||
| tColumn_3 | int | Which column of the template file corresponds to template #3 | ||||
| tColumn_4 | int | Which column of the template file corresponds to template #4 | ||||
| tColumn_5 | int | Which column of the template file corresponds to template #5 | ||||
| tColumn_6 | int | Which column of the template file corresponds to template #6 | ||||
| tColumn_7 | int | Which column of the template file corresponds to template #7 | ||||
| tColumn_8 | int | Which column of the template file corresponds to template #8 | ||||
| tColumn_9 | int | Which column of the template file corresponds to template #9 | ||||
| nPoly | float | Number of polynomial terms used in the fit | ||||
| theta_0 | float | Coefficient for template #0 of fit | ||||
| theta_1 | float | Coefficient for template #1 of fit | ||||
| theta_2 | float | Coefficient for template #2 of fit | ||||
| theta_3 | float | Coefficient for template #3 of fit | ||||
| theta_4 | float | Coefficient for template #4 of fit | ||||
| theta_5 | float | Coefficient for template #5 of fit | ||||
| theta_6 | float | Coefficient for template #6 of fit | ||||
| theta_7 | float | Coefficient for template #7 of fit | ||||
| theta_8 | float | Coefficient for template #8 of fit | ||||
| theta_9 | float | Coefficient for template #9 of fit | ||||
| velDisp | float | km/s | Velocity dispersion | |||
| velDispErr | float | km/s | Error in velocity dispersion | |||
| velDispZ | float | Redshift associated with best fit velocity dispersion | ||||
| velDispZErr | float | Error in redshift associated with best fit velocity dispersion | ||||
| velDispChi2 | float | Chi-squared associated with velocity dispersion fit | ||||
| velDispNPix | int | Number of pixels overlapping best template in velocity dispersion fit | ||||
| velDispDOF | int | Number of degrees of freedom in velocity dispersion fit | ||||
| waveMin | float | Angstroms | Minimum observed (vacuum) wavelength | |||
| waveMax | float | Angstroms | Maximum observed (vacuum) wavelength | |||
| wCoverage | float | Coverage in wavelength, in units of log10 wavelength | ||||
| snMedian_u | float | Median signal-to-noise over all good pixels in u-band | ||||
| snMedian_g | float | Median signal-to-noise over all good pixels in g-band | ||||
| snMedian_r | float | Median signal-to-noise over all good pixels in r-band | ||||
| snMedian_i | float | Median signal-to-noise over all good pixels in i-band | ||||
| snMedian_z | float | Median signal-to-noise over all good pixels in z-band | ||||
| snMedian | float | Median signal-to-noise over all good pixels | ||||
| chi68p | float | 68-th percentile value of abs(chi) of the best-fit synthetic spectrum to the actual spectrum (around 1.0 for a good fit) | ||||
| fracNSigma_1 | float | Fraction of pixels deviant by more than 1 sigma relative to best-fit | ||||
| fracNSigma_2 | float | Fraction of pixels deviant by more than 2 sigma relative to best-fit | ||||
| fracNSigma_3 | float | Fraction of pixels deviant by more than 3 sigma relative to best-fit | ||||
| fracNSigma_4 | float | Fraction of pixels deviant by more than 4 sigma relative to best-fit | ||||
| fracNSigma_5 | float | Fraction of pixels deviant by more than 5 sigma relative to best-fit | ||||
| fracNSigma_6 | float | Fraction of pixels deviant by more than 6 sigma relative to best-fit | ||||
| fracNSigma_7 | float | Fraction of pixels deviant by more than 7 sigma relative to best-fit | ||||
| fracNSigma_8 | float | Fraction of pixels deviant by more than 8 sigma relative to best-fit | ||||
| fracNSigma_9 | float | Fraction of pixels deviant by more than 9 sigma relative to best-fit | ||||
| fracNSigma_10 | float | Fraction of pixels deviant by more than 10 sigma relative to best-fit | ||||
| fracNSigHi_1 | float | Fraction of pixels high by more than 1 sigma relative to best-fit | ||||
| fracNSigHi_2 | float | Fraction of pixels high by more than 2 sigma relative to best-fit | ||||
| fracNSigHi_3 | float | Fraction of pixels high by more than 3 sigma relative to best-fit | ||||
| fracNSigHi_4 | float | Fraction of pixels high by more than 4 sigma relative to best-fit | ||||
| fracNSigHi_5 | float | Fraction of pixels high by more than 5 sigma relative to best-fit | ||||
| fracNSigHi_6 | float | Fraction of pixels high by more than 6 sigma relative to best-fit | ||||
| fracNSigHi_7 | float | Fraction of pixels high by more than 7 sigma relative to best-fit | ||||
| fracNSigHi_8 | float | Fraction of pixels high by more than 8 sigma relative to best-fit | ||||
| fracNSigHi_9 | float | Fraction of pixels high by more than 9 sigma relative to best-fit | ||||
| fracNSigHi_10 | float | Fraction of pixels high by more than 10 sigma relative to best-fit | ||||
| fracNSigLo_1 | float | Fraction of pixels low by more than 1 sigma relative to best-fit | ||||
| fracNSigLo_2 | float | Fraction of pixels low by more than 2 sigma relative to best-fit | ||||
| fracNSigLo_3 | float | Fraction of pixels low by more than 3 sigma relative to best-fit | ||||
| fracNSigLo_4 | float | Fraction of pixels low by more than 4 sigma relative to best-fit | ||||
| fracNSigLo_5 | float | Fraction of pixels low by more than 5 sigma relative to best-fit | ||||
| fracNSigLo_6 | float | Fraction of pixels low by more than 6 sigma relative to best-fit | ||||
| fracNSigLo_7 | float | Fraction of pixels low by more than 7 sigma relative to best-fit | ||||
| fracNSigLo_8 | float | Fraction of pixels low by more than 8 sigma relative to best-fit | ||||
| fracNSigLo_9 | float | Fraction of pixels low by more than 9 sigma relative to best-fit | ||||
| fracNSigLo_10 | float | Fraction of pixels low by more than 10 sigma relative to best-fit | ||||
| spectroFlux_u | float | nanomaggies | Spectrum projected onto u filter | |||
| spectroFlux_g | float | nanomaggies | Spectrum projected onto g filter | |||
| spectroFlux_r | float | nanomaggies | Spectrum projected onto r filter | |||
| spectroFlux_i | float | nanomaggies | Spectrum projected onto i filter | |||
| spectroFlux_z | float | nanomaggies | Spectrum projected onto z filter | |||
| spectroSynFlux_u | float | nanomaggies | Best-fit template spectrum projected onto u filter | |||
| spectroSynFlux_g | float | nanomaggies | Best-fit template spectrum projected onto g filter | |||
| spectroSynFlux_r | float | nanomaggies | Best-fit template spectrum projected onto r filter | |||
| spectroSynFlux_i | float | nanomaggies | Best-fit template spectrum projected onto i filter | |||
| spectroSynFlux_z | float | nanomaggies | Best-fit template spectrum projected onto z filter | |||
| spectroFluxIvar_u | float | nanomaggies | Inverse variance of spectrum projected onto u filter | |||
| spectroFluxIvar_g | float | nanomaggies | Inverse variance of spectrum projected onto g filter | |||
| spectroFluxIvar_r | float | nanomaggies | Inverse variance of spectrum projected onto r filter | |||
| spectroFluxIvar_i | float | nanomaggies | Inverse variance of spectrum projected onto i filter | |||
| spectroFluxIvar_z | float | nanomaggies | Inverse variance of spectrum projected onto z filter | |||
| spectroSynFluxIvar_u | float | nanomaggies | Inverse variance of best-fit template spectrum projected onto u filter | |||
| spectroSynFluxIvar_g | float | nanomaggies | Inverse variance of best-fit template spectrum projected onto g filter | |||
| spectroSynFluxIvar_r | float | nanomaggies | Inverse variance of best-fit template spectrum projected onto r filter | |||
| spectroSynFluxIvar_i | float | nanomaggies | Inverse variance of best-fit template spectrum projected onto i filter | |||
| spectroSynFluxIvar_z | float | nanomaggies | Inverse variance of best-fit template spectrum projected onto z filter | |||
| spectroSkyFlux_u | float | nanomaggies | Sky spectrum projected onto u filter | |||
| spectroSkyFlux_g | float | nanomaggies | Sky spectrum projected onto g filter | |||
| spectroSkyFlux_r | float | nanomaggies | Sky spectrum projected onto r filter | |||
| spectroSkyFlux_i | float | nanomaggies | Sky spectrum projected onto i filter | |||
| spectroSkyFlux_z | float | nanomaggies | Sky spectrum projected onto z filter | |||
| anyAndMask | int | For each bit, records whether any pixel in the spectrum has that bit set in its ANDMASK | ||||
| anyOrMask | int | For each bit, records whether any pixel in the spectrum has that bit set in its ORMASK | ||||
| plateSN2 | float | Overall signal-to-noise-squared measure for plate (only set for SDSS spectrograph) | ||||
| deredSN2 | float | Dereddened signal-to-noise-squared measure for plate (only set for BOSS spectrograph) | ||||
| snTurnoff | float | Signal to noise measure for MS turnoff stars on plate (-9999 if not appropriate) | ||||
| sn1_g | float | (S/N)^2 at g=20.20 for spectrograph #1 | ||||
| sn1_r | float | (S/N)^2 at r=20.25 for spectrograph #1 | ||||
| sn1_i | float | (S/N)^2 at i=19.90 for spectrograph #1 | ||||
| sn2_g | float | (S/N)^2 at g=20.20 for spectrograph #2 | ||||
| sn2_r | float | (S/N)^2 at r=20.25 for spectrograph #2 | ||||
| sn2_i | float | (S/N)^2 at i=19.90 for spectrograph #2 | ||||
| elodieFileName | string | File name for best-fit Elodie star | ||||
| elodieObject | string | Star name (mostly Henry Draper names) | ||||
| elodieSpType | string | Spectral type | ||||
| elodieBV | float | mag | (B-V) color | |||
| elodieTEff | float | Kelvin | Effective temperature | |||
| elodieLogG | float | log10(gravity) | ||||
| elodieFeH | float | Metallicity ([Fe/H]) | ||||
| elodieZ | float | Redshift | ||||
| elodieZErr | float | Redshift error (negative for invalid fit) | ||||
| elodieZModelErr | float | Standard deviation in redshift among the 12 best-fit stars | ||||
| elodieRChi2 | float | Reduced chi^2 | ||||
| elodieDOF | float | Degrees of freedom for fit | ||||
| htmID | long | 20 deep Hierarchical Triangular Mesh ID | ||||
| loadVersion | int | Load Version | ||||
| img | int | Spectrum Image | ||||
| sdssPrimary | int | Best version of spectrum at this location among SDSS plates |
The combined spectro and photo parameters of an object in SpecObjAl
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| specObjID | long | Unique ID | ||||
| mjd | int | MJD | MJD of observation | |||
| plate | int | Plate ID | ||||
| tile | int | Tile ID | ||||
| fiberID | int | Fiber ID | ||||
| z | float | Final Redshift | ||||
| zErr | float | Redshift error | ||||
| class | string | Spectroscopic class (GALAXY, QSO, or STAR) | ||||
| subClass | string | Spectroscopic subclass | ||||
| zWarning | int | Warning Flags | ||||
| ra | double | deg | ra in J2000 from SpecObj | |||
| dec | double | deg | dec in J2000 from SpecObj | |||
| cx | double | x of Normal unit vector in J2000 | ||||
| cy | double | y of Normal unit vector in J2000 | ||||
| cz | double | z of Normal unit vector in J2000 | ||||
| htmID | long | 20 deep Hierarchical Triangular Mesh ID | ||||
| sciencePrimary | int | Best version of spectrum at this location (defines default view SpecObj) | ||||
| legacyPrimary | int | Best version of spectrum at this location, among Legacy plates | ||||
| seguePrimary | int | Best version of spectrum at this location, among SEGUE plates (defines default view SpecObj) | ||||
| segue1Primary | int | Best version of spectrum at this location, among SEGUE-1 plates | ||||
| segue2Primary | int | Best version of spectrum at this location, among SEGUE-1 plates | ||||
| bossPrimary | int | Best version of spectrum at this location, among BOSS plates | ||||
| sdssPrimary | int | Best version of spectrum at this location among SDSS plates | ||||
| survey | string | Survey name | ||||
| programname | string | Program name | ||||
| legacy_target1 | long | for Legacy program, target selection information at plate design | ||||
| legacy_target2 | long | for Legacy program target selection information at plate design, secondary/qa/calibration | ||||
| special_target1 | long | for Special program target selection information at plate design | ||||
| special_target2 | long | for Special program target selection information at plate design, secondary/qa/calibration | ||||
| segue1_target1 | long | SEGUE-1 target selection information at plate design, primary science selection | ||||
| segue1_target2 | long | SEGUE-1 target selection information at plate design, secondary/qa/calib selection | ||||
| segue2_target1 | long | SEGUE-2 target selection information at plate design, primary science selection | ||||
| segue2_target2 | long | SEGUE-2 target selection information at plate design, secondary/qa/calib selection | ||||
| boss_target1 | long | BOSS target selection information at plate | ||||
| ancillary_target1 | long | BOSS ancillary science target selection information at plate design | ||||
| ancillary_target2 | long | BOSS ancillary target selection information at plate design | ||||
| plateID | long | Link to plate on which the spectrum was taken | ||||
| sourceType | string | type of object targeted as | ||||
| targetObjID | long | ID of target PhotoObj | ||||
| objID | long | Unique SDSS identifier composed from [skyVersion,rerun,run,camcol,field,obj]. | ||||
| skyVersion | int | 0 = OPDB target, 1 = OPDB best | ||||
| run | int | Run number | ||||
| rerun | int | Rerun number | ||||
| camcol | int | Camera column | ||||
| field | int | Field number | ||||
| obj | int | The object id within a field. Usually changes between reruns of the same field. | ||||
| mode | int | 1: primary, 2: secondary, 3: family object. | ||||
| nChild | int | Number of children if this is a deblened composite object. BRIGHT (in a flags sense) objects also have nchild==1, the non-BRIGHT sibling. | ||||
| type | int | Morphological type classification of the object. | ||||
| flags | long | Photo Object Attribute Flags | ||||
| psfMag_u | float | mag | PSF flux | |||
| psfMag_g | float | mag | PSF flux | |||
| psfMag_r | float | mag | PSF flux | |||
| psfMag_i | float | mag | PSF flux | |||
| psfMag_z | float | mag | PSF flux | |||
| psfMagErr_u | float | mag | PSF flux error | |||
| psfMagErr_g | float | mag | PSF flux error | |||
| psfMagErr_r | float | mag | PSF flux error | |||
| psfMagErr_i | float | mag | PSF flux error | |||
| psfMagErr_z | float | mag | PSF flux error | |||
| fiberMag_u | float | mag | Flux in 3 arcsec diameter fiber radius | |||
| fiberMag_g | float | mag | Flux in 3 arcsec diameter fiber radius | |||
| fiberMag_r | float | mag | Flux in 3 arcsec diameter fiber radius | |||
| fiberMag_i | float | mag | Flux in 3 arcsec diameter fiber radius | |||
| fiberMag_z | float | mag | Flux in 3 arcsec diameter fiber radius | |||
| fiberMagErr_u | float | mag | Flux in 3 arcsec diameter fiber radius error | |||
| fiberMagErr_g | float | mag | Flux in 3 arcsec diameter fiber radius error | |||
| fiberMagErr_r | float | mag | Flux in 3 arcsec diameter fiber radius error | |||
| fiberMagErr_i | float | mag | Flux in 3 arcsec diameter fiber radius error | |||
| fiberMagErr_z | float | mag | Flux in 3 arcsec diameter fiber radius error | |||
| petroMag_u | float | mag | Petrosian flux | |||
| petroMag_g | float | mag | Petrosian flux | |||
| petroMag_r | float | mag | Petrosian flux | |||
| petroMag_i | float | mag | Petrosian flux | |||
| petroMag_z | float | mag | Petrosian flux | |||
| petroMagErr_u | float | mag | Petrosian flux error | |||
| petroMagErr_g | float | mag | Petrosian flux error | |||
| petroMagErr_r | float | mag | Petrosian flux error | |||
| petroMagErr_i | float | mag | Petrosian flux error | |||
| petroMagErr_z | float | mag | Petrosian flux error | |||
| modelMag_u | float | mag | better of DeV/Exp magnitude fit | |||
| modelMag_g | float | mag | better of DeV/Exp magnitude fit | |||
| modelMag_r | float | mag | better of DeV/Exp magnitude fit | |||
| modelMag_i | float | mag | better of DeV/Exp magnitude fit | |||
| modelMag_z | float | mag | better of DeV/Exp magnitude fit | |||
| modelMagErr_u | float | mag | better of DeV/Exp magnitude fit error | |||
| modelMagErr_g | float | mag | better of DeV/Exp magnitude fit error | |||
| modelMagErr_r | float | mag | better of DeV/Exp magnitude fit error | |||
| modelMagErr_i | float | mag | better of DeV/Exp magnitude fit error | |||
| modelMagErr_z | float | mag | better of DeV/Exp magnitude fit error | |||
| cModelMag_u | float | mag | DeV+Exp magnitude | |||
| cModelMag_g | float | mag | DeV+Exp magnitude | |||
| cModelMag_r | float | mag | DeV+Exp magnitude | |||
| cModelMag_i | float | mag | DeV+Exp magnitude | |||
| cModelMag_z | float | mag | DeV+Exp magnitude | |||
| cModelMagErr_u | float | mag | DeV+Exp magnitude error | |||
| cModelMagErr_g | float | mag | DeV+Exp magnitude error | |||
| cModelMagErr_r | float | mag | DeV+Exp magnitude error | |||
| cModelMagErr_i | float | mag | DeV+Exp magnitude error | |||
| cModelMagErr_z | float | mag | DeV+Exp magnitude error | |||
| mRrCc_r | float | Adaptive (<r^2> + <c^2>) | ||||
| mRrCcErr_r | float | Error in adaptive (<r^2> + <c^2>) | ||||
| score | float | Quality of field (0-1) | ||||
| resolveStatus | int | Resolve status of object | ||||
| calibStatus_u | int | Calibration status in u-band | ||||
| calibStatus_g | int | Calibration status in g-band | ||||
| calibStatus_r | int | Calibration status in r-band | ||||
| calibStatus_i | int | Calibration status in i-band | ||||
| calibStatus_z | int | Calibration status in z-band | ||||
| photoRa | double | deg | J2000 right ascension (r') from Best | |||
| photoDec | double | deg | J2000 declination (r') from Best | |||
| extinction_u | float | mag | Reddening in each filter | |||
| extinction_g | float | mag | Reddening in each filter | |||
| extinction_r | float | mag | Reddening in each filter | |||
| extinction_i | float | mag | Reddening in each filter | |||
| extinction_z | float | mag | Reddening in each filter | |||
| fieldID | long | Link to the field this object is in | ||||
| dered_u | float | mag | Simplified mag, corrected for reddening: modelMag-reddening | |||
| dered_g | float | mag | Simplified mag, corrected for reddening: modelMag-reddening | |||
| dered_r | float | mag | Simplified mag, corrected for reddening: modelMag-reddening | |||
| dered_i | float | mag | Simplified mag, corrected for reddening: modelMag-reddening | |||
| dered_z | float | mag | Simplified mag, corrected for reddening: modelMag-reddening |
This table contains the definitions of the survey layout as planne
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| stripe | int | Stripe number | ||||
| hemisphere | string | Which hemisphere (N|S) | ||||
| eta | double | deg | Survey eta for the center of stripe | |||
| lambdaMin | double | deg | Survey lambda lower limit of the stripe | |||
| lambdaMax | double | deg | Survey lambda upper limit of the stripe | |||
| htmArea | string | HTM area descriptor string |
Keeps track of objects chosen by target selection and need to be tiled
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| targetID | long | hash of run, rerun, camcol, field, object (skyVersion=0) | ||||
| run | int | imaging run | ||||
| rerun | int | rerun number | ||||
| camcol | int | imaging camcol | ||||
| field | int | imaging field | ||||
| obj | int | imaging object id | ||||
| regionID | int | ID of sector, 0 if unset | ||||
| ra | double | deg | right ascension | |||
| dec | double | deg | declination | |||
| duplicate | int | duplicate spectrum by mistake | ||||
| htmID | long | htm index | ||||
| cx | double | x projection of vector on unit sphere | ||||
| cy | double | y projection of vector on unit sphere | ||||
| cz | double | z projection of vector on unit sphere | ||||
| bestObjID | long | hashed ID of object in best version of the sky | ||||
| specObjID | long | hashed ID of specobj in best version of the sky | ||||
| bestMode | int | mode from BEST PhotoObj | ||||
| loadVersion | int | Load Version |
Unique information for an object every time it is targette
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| targetObjID | long | ID of object in Target (foreign key to Target.TargetObjID) | ||||
| targetID | long | ID of entry in Target table | ||||
| skyVersion | int | skyVersion | ||||
| primTarget | int | primTarget from TARGET | ||||
| secTarget | int | secTarget from TARGET | ||||
| priority | int | target selection priority | ||||
| programType | int | spectroscopic program type | ||||
| programName | string | character string of program (from plate inventory db) | ||||
| targetMode | int | mode from TARGET PhotoObj | ||||
| loadVersion | int | Load Version |
2MASS point-source catalog quantities for matches to SDSS photometr
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| objID | long | Unique SDSS identifier composed from [skyVersion,rerun,run,camcol,field,obj]. | ||||
| ra | double | deg | 2MASS right ascension, J2000 | |||
| dec | double | deg | 2MASS declination, J2000 | |||
| errMaj | float | arcsec | Semi-major axis length of the one sigma position uncertainty ellipse | |||
| errMin | float | arcsec | Semi-minor axis length of the one sigma position uncertainty ellipse | |||
| errAng | float | deg | Position angle on the sky of the semi-major axis of the position uncertainty ellipse (East of North) | |||
| j | float | mag | default J-band apparent magnitude (Vega relative, no Galactic extinction correction | |||
| jIvar | float | inverse mag^2 | inverse variance in J-band apparent magnitude | |||
| h | float | mag | default H-band apparent magnitude (Vega relative, no Galactic extinction correction | |||
| hIvar | float | inverse mag^2 | inverse variance in H-band apparent magnitude | |||
| k | float | mag | default K-band apparent magnitude (Vega relative, no Galactic extinction correction | |||
| kIvar | float | inverse mag^2 | inverse variance in K-band apparent magnitude | |||
| phQual | string | photometric quality flag (see 2MASS PSC documentation) | ||||
| rdFlag | string | Read flag. Three character flag, one character per band [JHKs], that indicates the origin of the default magnitudes and uncertainties in each band (see 2MASS PSC documentation) | ||||
| blFlag | string | Blend flag. Three character flag, one character per band [JHKs], that indicates the number of components that were fit simultaneously when estimating the brightness of a source (see 2MASS PSC documentation) | ||||
| ccFlag | string | Contamination and confusion flag. Three character flag, one character per band [JHKs], that indicates that the photometry and/or position measurements of a source may be contaminated or biased due to proximity to an image artifact or nearby source of equal or greater brightness. (See 2MASS PSC documentation). | ||||
| nDetectJ | int | Number of frames on which 2MASS source was detected in J-band | ||||
| nDetectH | int | Number of frames on which 2MASS source was detected in H-band | ||||
| nDetectK | int | Number of frames on which 2MASS source was detected in K-band | ||||
| nObserveJ | int | Number of frames which 2MASS source was within the boundaries of in J-band | ||||
| nObserveH | int | Number of frames which 2MASS source was within the boundaries of in H-band | ||||
| nObserveK | int | Number of frames which 2MASS source was within the boundaries of in K-band | ||||
| galContam | int | Extended source "contamination" flag. A value of gal_contam="0" indicates no contamination. "1" indicates it is probably an extended source itself (this does not detect all such cases!). "2" indicates it is within the boundary of a large XSC source. (See 2MASS PSC documentation). | ||||
| mpFlag | int | Minor planet flag. "1" if source associated with known solar system object, "0" otherwise. (See 2MASS PSC documentation). | ||||
| ptsKey | int | Unique identification number for the PSC source. | ||||
| hemis | string | Hemisphere code for the 2MASS Observatory from which this source was observed. "n" means North (Mt. Hopkins); "s" means South (CTIO). | ||||
| jDate | double | Julian Date of the source measurement accurate to +30 seconds. (See 2MASS PSC documentation). | ||||
| dupSource | int | Duplicate source flag. Used in conjunction with the use_src flag, this numerical flag indicates whether the source falls in a Tile overlap region, and if so, if it was detected multiple times. (See 2MASS PSC documentation) | ||||
| useSource | int | Use source flag. Used in conjunction with the dup_src flag, this numerical flag indicates if a source falls within a Tile overlap region, and whether or not it satisfies the unbiased selection rules for multiple source resolution. (See 2MASS PSC documentation). |
2MASS extended-source catalog quantities for matches to SDSS photometr
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| objID | long | Unique SDSS identifier composed from [skyVersion,rerun,run,camcol,field,obj]. | ||||
| tmassxsc_ra | double | deg | 2MASS right ascension, J2000 | |||
| tmassxsc_dec | double | deg | 2MASS declination, J2000 | |||
| jDate | double | Julian Date of the source measurement accurate to +30 seconds. (See 2MASS PSC documentation). | ||||
| designation | string | Sexagesimal, equatorial position-based source name in the form: hhmmssss+ddmmsss[ABC...]. | ||||
| sup_ra | double | Super-coadd centroid RA (J2000 decimal deg). | ||||
| sup_dec | double | Super-coadd centroid Dec (J2000 decimal deg). | ||||
| density | float | Coadd log(density) of stars with k<14 mag. | ||||
| R_K20FE | float | mag | 20mag/sq arcsec isophotal K fiducial ell. ap. semi-major axis. | |||
| J_M_K20FE | float | mag | J 20mag/sq arcsec isophotal fiducial ell. ap. magnitude. | |||
| J_MSIG_K20FE | float | mag | J 1-sigma uncertainty in 20mag/sq arcsec iso.fid.ell.mag. | |||
| J_FLG_K20FE | int | J confusion flag for 20mag/sq arcsec iso. fid. ell. mag. | ||||
| H_M_K20FE | float | mag | H 20mag/sq arcsec isophotal fiducial ell. ap. magnitude. | |||
| H_MSIG_K20FE | float | mag | H 1-sigma uncertainty in 20mag/sq arcsec iso.fid.ell.mag. | |||
| H_FLG_K20FE | int | H confusion flag for 20mag/sq arcsec iso. fid. ell. mag. | ||||
| K_M_K20FE | float | mag | K 20mag/sq arcsec isophotal fiducial ell. ap. magnitude. | |||
| K_MSIG_K20FE | float | mag | K 1-sigma uncertainty in 20mag/sq arcsec iso.fid.ell.mag. | |||
| K_FLG_K20FE | int | K confusion flag for 20mag/sq arcsec iso. fid. ell. mag. | ||||
| R_3SIG | float | arcsec | 3-sigma K isophotal semi-major axis. | |||
| J_BA | float | J minor/major axis ratio fit to the 3-sigma isophote. | ||||
| J_PHI | int | deg | J angle to 3-sigma major axis (E of N). | |||
| H_BA | float | H minor/major axis ratio fit to the 3-sigma isophote. | ||||
| H_PHI | int | deg | H angle to 3-sigma major axis (E of N). | |||
| K_BA | float | K minor/major axis ratio fit to the 3-sigma isophote. | ||||
| K_PHI | int | deg | K angle to 3-sigma major axis (E of N). | |||
| SUP_R_3SIG | float | Super-coadd minor/major axis ratio fit to the 3-sigma isophote. | ||||
| SUP_BA | float | K minor/major axis ratio fit to the 3-sigma isophote. | ||||
| SUP_PHI | int | deg | K angle to 3-sigma major axis (E of N). | |||
| R_FE | float | K fiducial Kron elliptical aperture semi-major axis. | ||||
| J_M_FE | float | mag | J fiducial Kron elliptical aperture magnitude. | |||
| J_MSIG_FE | float | mag | J 1-sigma uncertainty in fiducial Kron ell. mag. | |||
| J_FLG_FE | int | J confusion flag for fiducial Kron ell. mag. | ||||
| H_M_FE | float | mag | H fiducial Kron elliptical aperture magnitude. | |||
| H_MSIG_FE | float | mag | H 1-sigma uncertainty in fiducial Kron ell. mag. | |||
| H_FLG_FE | int | H confusion flag for fiducial Kron ell. mag. | ||||
| K_M_FE | float | mag | K fiducial Kron elliptical aperture magnitude. | |||
| K_MSIG_FE | float | mag | K 1-sigma uncertainty in fiducial Kron ell. mag. | |||
| K_FLG_FE | int | K confusion flag for fiducial Kron ell. mag. | ||||
| R_EXT | float | arcsec | extrapolation/total radius. | |||
| J_M_EXT | float | mag | J mag from fit extrapolation. | |||
| J_MSIG_EXT | float | mag | J 1-sigma uncertainty in mag from fit extrapolation. | |||
| J_PCHI | float | J chi^2 of fit to rad. profile | ||||
| H_M_EXT | float | mag | H mag from fit extrapolation. | |||
| H_MSIG_EXT | float | mag | H 1-sigma uncertainty in mag from fit extrapolation. | |||
| H_PCHI | float | H chi^2 of fit to rad. profile | ||||
| K_M_EXT | float | mag | K mag from fit extrapolation. | |||
| K_MSIG_EXT | float | mag | K 1-sigma uncertainty in mag from fit extrapolation. | |||
| K_PCHI | float | K chi^2 of fit to rad. profile | ||||
| J_R_EFF | float | arcsec | J half-light (integrated half-flux point) radius. | |||
| J_MNSURFB_EFF | float | mag/sq. arcsec | J mean surface brightness at the half-light radius. | |||
| H_R_EFF | float | arcsec | H half-light (integrated half-flux point) radius. | |||
| H_MNSURFB_EFF | float | mag/sq. arcsec | H mean surface brightness at the half-light radius. | |||
| K_R_EFF | float | arcsec | K half-light (integrated half-flux point) radius. | |||
| K_MNSURFB_EFF | float | mag/sq. arcsec | K mean surface brightness at the half-light radius. | |||
| J_CON_INDX | float | J concentration index r_75%/r_25%. | ||||
| H_CON_INDX | float | H concentration index r_75%/r_25%. | ||||
| K_CON_INDX | float | K concentration index r_75%/r_25%. | ||||
| J_PEAK | float | mag/sq. arcsec | J peak pixel brightness. | |||
| H_PEAK | float | mag/sq. arcsec | H peak pixel brightness. | |||
| K_PEAK | float | mag/sq. arcsec | K peak pixel brightness. | |||
| J_5SURF | float | mag/sq. arcsec | J central surface brightness (r<=5). | |||
| H_5SURF | float | mag/sq. arcsec | H central surface brightness (r<=5). | |||
| K_5SURF | float | mag/sq. arcsec | K central surface brightness (r<=5). | |||
| E_SCORE | float | extended score: 1(extended) < e_score < 2(point-like). | ||||
| G_SCORE | float | galaxy score: 1(extended) < g_score < 2(point-like). | ||||
| VC | int | visual verification score for source. | ||||
| CC_FLG | string | indicates artifact contamination and/or confusion. | ||||
| IM_NX | int | size of postage stamp image in pixels. | ||||
| R_K20FC | float | arcsec | 20mag/sq arcsec isophotal K fiducial circular ap. radius. | |||
| J_M_K20FC | float | mag | J 20mag/sq arcsec isophotal fiducial circ. ap. mag. | |||
| J_MSIG_K20FC | float | mag | J 1-sigma uncertainty in 20mag/sq arcsec iso.fid.circ. mag. | |||
| J_FLG_K20FC | int | J confusion flag for 20mag/sq arcsec iso. fid. circ. mag. | ||||
| H_M_K20FC | float | mag | H 20mag/sq arcsec isophotal fiducial circ. ap. mag. | |||
| H_MSIG_K20FC | float | mag | H 1-sigma uncertainty in 20mag/sq arcsec iso.fid.circ. mag. | |||
| H_FLG_K20FC | int | H confusion flag for 20mag/sq arcsec iso. fid. circ. mag. | ||||
| K_M_K20FC | float | mag | K 20mag/sq arcsec isophotal fiducial circ. ap. mag. | |||
| K_MSIG_K20FC | float | mag | K 1-sigma uncertainty in 20mag/sq arcsec iso.fid.circ. mag. | |||
| K_FLG_K20FC | int | K confusion flag for 20mag/sq arcsec iso. fid. circ. mag. | ||||
| J_R_E | float | arcsec | J Kron elliptical aperture semi-major axis. | |||
| J_M_E | float | mag | J Kron elliptical aperture magnitude | |||
| J_MSIG_E | float | mag | J 1-sigma uncertainty in Kron elliptical mag. | |||
| J_FLG_E | int | J confusion flag for Kron elliptical mag. | ||||
| H_R_E | float | arcsec | H Kron elliptical aperture semi-major axis. | |||
| H_M_E | float | mag | H Kron elliptical aperture magnitude | |||
| H_MSIG_E | float | mag | H 1-sigma uncertainty in Kron elliptical mag. | |||
| H_FLG_E | int | H confusion flag for Kron elliptical mag. | ||||
| K_R_E | float | arcsec | K Kron elliptical aperture semi-major axis. | |||
| K_M_E | float | mag | K Kron elliptical aperture magnitude | |||
| K_MSIG_E | float | mag | K 1-sigma uncertainty in Kron elliptical mag. | |||
| K_FLG_E | int | K confusion flag for Kron elliptical mag. | ||||
| J_R_C | float | arcsec | J Kron circular aperture radius. | |||
| J_M_C | float | mag | J Kron circular aperture magnitude. | |||
| J_MSIG_C | float | mag | J 1-sigma uncertainty in Kron circular mag. | |||
| J_FLG_C | int | J confusion flag for Kron circular mag. | ||||
| H_R_C | float | arcsec | H Kron circular aperture radius. | |||
| H_M_C | float | mag | H Kron circular aperture magnitude. | |||
| H_MSIG_C | float | mag | H 1-sigma uncertainty in Kron circular mag. | |||
| H_FLG_C | int | H confusion flag for Kron circular mag. | ||||
| K_R_C | float | arcsec | K Kron circular aperture radius. | |||
| K_M_C | float | mag | K Kron circular aperture magnitude. | |||
| K_MSIG_C | float | mag | K 1-sigma uncertainty in Kron circular mag. | |||
| K_FLG_C | int | K confusion flag for Kron circular mag. | ||||
| R_FC | float | arcsec | K fiducial Kron circular aperture radius. | |||
| J_M_FC | float | mag | J fiducial Kron circular magnitude. | |||
| J_MSIG_FC | float | mag | J 1-sigma uncertainty in fiducial Kron circ. mag. | |||
| J_FLG_FC | int | J confusion flag for Kron circular mag. confusion flag for fiducial Kron circ. mag. | ||||
| H_M_FC | float | mag | H fiducial Kron circular magnitude. | |||
| H_MSIG_FC | float | mag | H 1-sigma uncertainty in fiducial Kron circ. mag. | |||
| H_FLG_FC | int | H confusion flag for Kron circular mag. confusion flag for fiducial Kron circ. mag. | ||||
| K_M_FC | float | mag | K fiducial Kron circular magnitude. | |||
| K_MSIG_FC | float | mag | K 1-sigma uncertainty in fiducial Kron circ. mag. | |||
| K_FLG_FC | int | K confusion flag for Kron circular mag. confusion flag for fiducial Kron circ. mag. | ||||
| J_R_I20E | float | arcsec | J 20mag/sq arcsec isophotal elliptical ap. semi-major axis. | |||
| J_M_I20E | float | mag | J 20mag/sq arcsec isophotal elliptical ap. magnitude. | |||
| J_MSIG_I20E | float | mag | J 1-sigma uncertainty in 20mag/sq arcsec iso. ell. mag. | |||
| J_FLG_I20E | int | J confusion flag for 20mag/sq arcsec iso. ell. mag. | ||||
| H_R_I20E | float | arcsec | H 20mag/sq arcsec isophotal elliptical ap. semi-major axis. | |||
| H_M_I20E | float | mag | H 20mag/sq arcsec isophotal elliptical ap. magnitude. | |||
| H_MSIG_I20E | float | mag | H 1-sigma uncertainty in 20mag/sq arcsec iso. ell. mag. | |||
| H_FLG_I20E | int | H confusion flag for 20mag/sq arcsec iso. ell. mag. | ||||
| K_R_I20E | float | arcsec | K 20mag/sq arcsec isophotal elliptical ap. semi-major axis. | |||
| K_M_I20E | float | mag | K 20mag/sq arcsec isophotal elliptical ap. magnitude. | |||
| K_MSIG_I20E | float | mag | K 1-sigma uncertainty in 20mag/sq arcsec iso. ell. mag. | |||
| K_FLG_I20E | int | K confusion flag for 20mag/sq arcsec iso. ell. mag. | ||||
| J_R_I20C | float | arcsec | J 20mag/sq arcsec isophotal circular aperture radius. | |||
| J_M_I20C | float | mag | J 20mag/sq arcsec isophotal circular ap. magnitude. | |||
| J_MSIG_I20C | float | mag | J 1-sigma uncertainty in 20mag/sq arcsec iso. circ. mag. | |||
| J_FLG_I20C | int | J confusion flag for 20mag/sq arcsec iso. circ. mag. | ||||
| H_R_I20C | float | arcsec | H 20mag/sq arcsec isophotal circular aperture radius. | |||
| H_M_I20C | float | mag | H 20mag/sq arcsec isophotal circular ap. magnitude. | |||
| H_MSIG_I20C | float | mag | H 1-sigma uncertainty in 20mag/sq arcsec iso. circ. mag. | |||
| H_FLG_I20C | int | H confusion flag for 20mag/sq arcsec iso. circ. mag. | ||||
| K_R_I20C | float | arcsec | K 20mag/sq arcsec isophotal circular aperture radius. | |||
| K_M_I20C | float | mag | K 20mag/sq arcsec isophotal circular ap. magnitude. | |||
| K_MSIG_I20C | float | mag | K 1-sigma uncertainty in 20mag/sq arcsec iso. circ. mag. | |||
| K_FLG_I20C | int | K confusion flag for 20mag/sq arcsec iso. circ. mag. | ||||
| J_R_I21E | float | arcsec | J 21mag/sq arcsec isophotal elliptical ap. semi-major axis. | |||
| J_M_I21E | float | mag | J 21mag/sq arcsec isophotal elliptical ap. magnitude. | |||
| J_MSIG_I21E | float | mag | J 1-sigma uncertainty in 21mag/sq arcsec iso. ell. mag. | |||
| J_FLG_I21E | int | J confusion flag for 21mag/sq arcsec iso. ell. mag. | ||||
| H_R_I21E | float | arcsec | H 21mag/sq arcsec isophotal elliptical ap. semi-major axis. | |||
| H_M_I21E | float | mag | H 21mag/sq arcsec isophotal elliptical ap. magnitude. | |||
| H_MSIG_I21E | float | mag | H 1-sigma uncertainty in 21mag/sq arcsec iso. ell. mag. | |||
| H_FLG_I21E | int | H confusion flag for 21mag/sq arcsec iso. ell. mag. | ||||
| K_R_I21E | float | arcsec | K 21mag/sq arcsec isophotal elliptical ap. semi-major axis. | |||
| K_M_I21E | float | mag | K 21mag/sq arcsec isophotal elliptical ap. magnitude. | |||
| K_MSIG_I21E | float | mag | K 1-sigma uncertainty in 21mag/sq arcsec iso. ell. mag. | |||
| K_FLG_I21E | int | K confusion flag for 21mag/sq arcsec iso. ell. mag. | ||||
| R_J21FE | float | |||||
| J_M_J21FE | float | mag | J 21mag/sq arcsec isophotal fiducial ell. ap. magnitude. | |||
| J_MSIG_J21FE | float | mag | J 1-sigma uncertainty in 21mag/sq arcsec iso.fid.ell.mag. | |||
| J_FLG_J21FE | int | J confusion flag for 21mag/sq arcsec iso. fid. ell. mag. | ||||
| H_M_J21FE | float | mag | H 21mag/sq arcsec isophotal fiducial ell. ap. magnitude. | |||
| H_MSIG_J21FE | float | mag | H 1-sigma uncertainty in 21mag/sq arcsec iso.fid.ell.mag. | |||
| H_FLG_J21FE | int | H confusion flag for 21mag/sq arcsec iso. fid. ell. mag. | ||||
| K_M_J21FE | float | mag | K 21mag/sq arcsec isophotal fiducial ell. ap. magnitude. | |||
| K_MSIG_J21FE | float | mag | K 1-sigma uncertainty in 21mag/sq arcsec iso.fid.ell.mag. | |||
| K_FLG_J21FE | int | K confusion flag for 21mag/sq arcsec iso. fid. ell. mag. | ||||
| J_R_I21C | float | arcsec | J 21mag/sq arcsec isophotal circular aperture radius. | |||
| J_M_I21C | float | mag | J 21mag/sq arcsec isophotal circular ap. magnitude. | |||
| J_MSIG_I21C | float | mag | J 1-sigma uncertainty in 21mag/sq arcsec iso. circ. mag. | |||
| J_FLG_I21C | int | J confusion flag for 21mag/sq arcsec iso. circ. mag. | ||||
| H_R_I21C | float | arcsec | H 21mag/sq arcsec isophotal circular aperture radius. | |||
| H_M_I21C | float | mag | H 21mag/sq arcsec isophotal circular ap. magnitude. | |||
| H_MSIG_I21C | float | mag | H 1-sigma uncertainty in 21mag/sq arcsec iso. circ. mag. | |||
| H_FLG_I21C | int | H confusion flag for 21mag/sq arcsec iso. circ. mag. | ||||
| K_R_I21C | float | arcsec | K 21mag/sq arcsec isophotal circular aperture radius. | |||
| K_M_I21C | float | mag | K 21mag/sq arcsec isophotal circular ap. magnitude. | |||
| K_MSIG_I21C | float | mag | K 1-sigma uncertainty in 21mag/sq arcsec iso. circ. mag. | |||
| K_FLG_I21C | int | K confusion flag for 21mag/sq arcsec iso. circ. mag. | ||||
| R_J21FC | float | arcsec | 21mag/sq arcsec isophotal J fiducial circular ap. radius. | |||
| J_M_J21FC | float | mag | J 21mag/sq arcsec isophotal fiducial circ. ap. mag. | |||
| J_MSIG_J21FC | float | mag | J 1-sigma uncertainty in 21mag/sq arcsec iso.fid.circ.mag. | |||
| J_FLG_J21FC | int | J confusion flag for 21mag/sq arcsec iso. fid. circ. mag. | ||||
| H_M_J21FC | float | mag | H 21mag/sq arcsec isophotal fiducial circ. ap. mag. | |||
| H_MSIG_J21FC | float | mag | H 1-sigma uncertainty in 21mag/sq arcsec iso.fid.circ.mag. | |||
| H_FLG_J21FC | int | H confusion flag for 21mag/sq arcsec iso. fid. circ. mag. | ||||
| K_M_J21FC | float | mag | K 21mag/sq arcsec isophotal fiducial circ. ap. mag. | |||
| K_MSIG_J21FC | float | mag | K 1-sigma uncertainty in 21mag/sq arcsec iso.fid.circ.mag. | |||
| K_FLG_J21FC | int | K confusion flag for 21mag/sq arcsec iso. fid. circ. mag. | ||||
| J_M_SYS | float | mag | J system photometry magnitude. | |||
| J_MSIG_SYS | float | mag | J 1-sigma uncertainty in system photometry mag. | |||
| H_M_SYS | float | mag | H system photometry magnitude. | |||
| H_MSIG_SYS | float | mag | H 1-sigma uncertainty in system photometry mag. | |||
| K_M_SYS | float | mag | K system photometry magnitude. | |||
| K_MSIG_SYS | float | mag | K 1-sigma uncertainty in system photometry mag. | |||
| SYS_FLG | int | system flag: 0=no system, 1=nearby galaxy flux incl. in mag. | ||||
| CONTAM_FLG | int | contamination flag: 0=no stars, 1=stellar flux incl. in mag. | ||||
| J_5SIG_BA | float | J minor/major axis ratio fit to the 5-sigma isophote. | ||||
| J_5SIG_PHI | int | deg | J angle to 5-sigma major axis (E of N). | |||
| H_5SIG_BA | float | H minor/major axis ratio fit to the 5-sigma isophote. | ||||
| H_5SIG_PHI | int | deg | H angle to 5-sigma major axis (E of N). | |||
| K_5SIG_BA | float | K minor/major axis ratio fit to the 5-sigma isophote. | ||||
| K_5SIG_PHI | int | deg | K angle to 5-sigma major axis (E of N). | |||
| J_D_AREA | int | sq arcsec | J 5-sigma to 3-sigma differential area. | |||
| J_PERC_DAREA | int | sq arcsec | J 5-sigma to 3-sigma percent area change. | |||
| H_D_AREA | int | sq arcsec | H 5-sigma to 3-sigma differential area. | |||
| H_PERC_DAREA | int | sq arcsec | H 5-sigma to 3-sigma percent area change. | |||
| K_D_AREA | int | sq arcsec | K 5-sigma to 3-sigma differential area. | |||
| K_PERC_DAREA | int | sq arcsec | K 5-sigma to 3-sigma percent area change. | |||
| J_BISYM_RAT | float | J bi-symmetric flux ratio. | ||||
| J_BISYM_CHI | float | J bi-symmetric cross-correlation chi. | ||||
| H_BISYM_RAT | float | H bi-symmetric flux ratio. | ||||
| H_BISYM_CHI | float | H bi-symmetric cross-correlation chi. | ||||
| K_BISYM_RAT | float | K bi-symmetric flux ratio. | ||||
| K_BISYM_CHI | float | K bi-symmetric cross-correlation chi. | ||||
| J_SH0 | float | J ridge shape (LCSB: BSNR limit). | ||||
| J_SIG_SH0 | float | J ridge shape sigma (LCSB: B2SNR limit). | ||||
| H_SH0 | float | H ridge shape (LCSB: BSNR limit). | ||||
| H_SIG_SH0 | float | H ridge shape sigma (LCSB: B2SNR limit). | ||||
| K_SH0 | float | K ridge shape (LCSB: BSNR limit). | ||||
| K_SIG_SH0 | float | K ridge shape sigma (LCSB: B2SNR limit). | ||||
| J_SC_MXDN | float | J mxdn (score) (LCSB: BSNR - block/smoothed SNR) | ||||
| J_SC_SH | float | J shape (score). | ||||
| J_SC_WSH | float | J wsh (score) (LCSB: PSNR - peak raw SNR). | ||||
| J_SC_R23 | float | J r23 (score) (LCSB: TSNR - integrated SNR for r=15). | ||||
| J_SC_1MM | float | J 1st moment (score) (LCSB: super blk 2,4,8 SNR). | ||||
| J_SC_2MM | float | J 2nd moment (score) (LCSB: SNRMAX - super SNR max). | ||||
| J_SC_VINT | float | J vint (score). | ||||
| J_SC_R1 | float | J r1 (score). | ||||
| J_SC_MSH | float | J median shape score. | ||||
| H_SC_MXDN | float | H mxdn (score) (LCSB: BSNR - block/smoothed SNR) | ||||
| H_SC_SH | float | H shape (score). | ||||
| H_SC_WSH | float | H wsh (score) (LCSB: PSNR - peak raw SNR). | ||||
| H_SC_R23 | float | H r23 (score) (LCSB: TSNR - integrated SNR for r=15). | ||||
| H_SC_1MM | float | H 1st moment (score) (LCSB: super blk 2,4,8 SNR). | ||||
| H_SC_2MM | float | H 2nd moment (score) (LCSB: SNRMAX - super SNR max). | ||||
| H_SC_VINT | float | H vint (score). | ||||
| H_SC_R1 | float | H r1 (score). | ||||
| H_SC_MSH | float | H median shape score. | ||||
| K_SC_MXDN | float | K mxdn (score) (LCSB: BSNR - block/smoothed SNR) | ||||
| K_SC_SH | float | K shape (score). | ||||
| K_SC_WSH | float | K wsh (score) (LCSB: PSNR - peak raw SNR). | ||||
| K_SC_R23 | float | K r23 (score) (LCSB: TSNR - integrated SNR for r=15). | ||||
| K_SC_1MM | float | K 1st moment (score) (LCSB: super blk 2,4,8 SNR). | ||||
| K_SC_2MM | float | K 2nd moment (score) (LCSB: SNRMAX - super SNR max). | ||||
| K_SC_VINT | float | K vint (score). | ||||
| K_SC_R1 | float | K r1 (score). | ||||
| K_SC_MSH | float | K median shape score. | ||||
| J_CHIF_ELLF | float | J % chi-fraction for elliptical fit to 3-sig isophote. | ||||
| K_CHIF_ELLF | float | K % chi-fraction for elliptical fit to 3-sig isophote. | ||||
| ELLFIT_FLG | int | ellipse fitting contamination flag. | ||||
| SUP_CHIF_ELLF | float | super-coadd % chi-fraction for ellip. fit to 3-sig isophote. | ||||
| N_BLANK | int | number of blanked source records. | ||||
| N_SUB | int | number of subtracted source records. | ||||
| BL_SUB_FLG | int | blanked/subtracted src description flag. | ||||
| ID_FLG | int | type/galaxy ID flag (0=non-catalog, 1=catalog, 2=LCSB). | ||||
| ID_CAT | string | matched galaxy catalog name. | ||||
| FG_FLG | string | flux-growth convergence flag. | ||||
| BLK_FAC | int | LCSB blocking factor (1, 2, 4, 8). | ||||
| DUP_SRC | int | Duplicate source flag. | ||||
| USE_SRC | int | Use source flag. | ||||
| PROX | float | arcsec | Proximity. The distance between this source and its nearest neighbor in the PSC. | |||
| PXPA | int | deg | The position angle on the sky of the vector from the source to the nearest neighbor in the PSC, East of North. | |||
| PXCNTR | int | ext_key value of nearest XSC source. | ||||
| DIST_EDGE_NS | int | The distance from the source to the nearest North or South scan edge. | ||||
| DIST_EDGE_EW | int | arcsec | The distance from the source to the nearest East or West scan edge. | |||
| DIST_EDGE_FLG | string | flag indicating which edges ([n|s][e|w]) are nearest to src. | ||||
| PTS_KEY | int | key to point source data DB record. | ||||
| MP_KEY | int | key to minor planet prediction DB record. | ||||
| NIGHT_KEY | int | key to night data record in "scan DB". | ||||
| SCAN_KEY | int | key to scan data record in "scan DB". | ||||
| COADD_KEY | int | key to coadd data record in "scan DB". | ||||
| HEMIS | string | hemisphere (N/S) of observation. "n" = North/Mt. Hopkins; "s" = South/CTIO. | ||||
| DATE | string | The observation reference date for this source expressed in ISO standard format. | ||||
| SCAN | int | scan number (unique within date). | ||||
| COADD | int | 3-digit coadd number (unique within scan). | ||||
| X_COADD | float | pix | x (cross-scan) position (coadd coord.). | |||
| Y_COADD | float | pix | y (in-scan) position (coadd coord.). | |||
| J_SUBST2 | float | J residual background #2 (score). | ||||
| H_SUBST2 | float | H residual background #2 (score). | ||||
| K_SUBST2 | float | K residual background #2 (score). | ||||
| J_BACK | float | mag/sq arcsec | J coadd median background. | |||
| H_BACK | float | mag/sq arcsec | H coadd median background. | |||
| K_BACK | float | mag/sq arcsec | K coadd median background. | |||
| J_RESID_ANN | float | mag/sq arcsec | J residual annulus background median. | |||
| H_RESID_ANN | float | mag/sq arcsec | H residual annulus background median. | |||
| K_RESID_ANN | float | mag/sq arcsec | K residual annulus background median. | |||
| J_BNDG_PER | int | J banding Fourier Transf. period on this side of coadd. | ||||
| J_BNDG_AMP | float | J banding maximum FT amplitude on this side of coadd. | ||||
| H_BNDG_PER | int | H banding Fourier Transf. period on this side of coadd. | ||||
| H_BNDG_AMP | float | H banding maximum FT amplitude on this side of coadd. | ||||
| K_BNDG_PER | int | K banding Fourier Transf. period on this side of coadd. | ||||
| K_BNDG_AMP | float | K banding maximum FT amplitude on this side of coadd. | ||||
| J_SEETRACK | float | J band seetracking score. | ||||
| H_SEETRACK | float | H band seetracking score. | ||||
| K_SEETRACK | float | K band seetracking score. | ||||
| EXT_KEY | int | entry counter (key) number (unique within table). | ||||
| TMASSXSC_ID | int | source ID number (unique within scan, coadd). | ||||
| J_M_5 | float | mag | J-band circular aperture magnitude (5 arcsec radius) | |||
| J_MSIG_5 | float | mag | error in J-band circular aperture magnitude (5 arcsec radius) | |||
| J_FLG_5 | int | J confusion flag for 5 arcsec circular ap. mag. | ||||
| J_M_7 | float | mag | J-band circular aperture magnitude (7 arcsec radius) | |||
| J_MSIG_7 | float | mag | error in J-band circular aperture magnitude (7 arcsec radius) | |||
| J_FLG_7 | int | J confusion flag for 7 arcsec circular ap. mag. | ||||
| J_M_10 | float | mag | J-band circular aperture magnitude (10 arcsec radius) | |||
| J_MSIG_10 | float | mag | error in J-band circular aperture magnitude (10 arcsec radius) | |||
| J_FLG_10 | int | J confusion flag for 10 arcsec circular ap. mag. | ||||
| J_M_15 | float | mag | J-band circular aperture magnitude (15 arcsec radius) | |||
| J_MSIG_15 | float | mag | error in J-band circular aperture magnitude (15 arcsec radius) | |||
| J_FLG_15 | int | J confusion flag for 15 arcsec circular ap. mag. | ||||
| J_M_20 | float | mag | J-band circular aperture magnitude (20 arcsec radius) | |||
| J_MSIG_20 | float | mag | error in J-band circular aperture magnitude (20 arcsec radius) | |||
| J_FLG_20 | int | J confusion flag for 20 arcsec circular ap. mag. | ||||
| J_M_25 | float | mag | J-band circular aperture magnitude (25 arcsec radius) | |||
| J_MSIG_25 | float | mag | error in J-band circular aperture magnitude (25 arcsec radius) | |||
| J_FLG_25 | int | J confusion flag for 25 arcsec circular ap. mag. | ||||
| J_M_30 | float | mag | J-band circular aperture magnitude (30 arcsec radius) | |||
| J_MSIG_30 | float | mag | error in J-band circular aperture magnitude (30 arcsec radius) | |||
| J_FLG_30 | int | J confusion flag for 30 arcsec circular ap. mag. | ||||
| J_M_40 | float | mag | J-band circular aperture magnitude (40 arcsec radius) | |||
| J_MSIG_40 | float | mag | error in J-band circular aperture magnitude (40 arcsec radius) | |||
| J_FLG_40 | int | J confusion flag for 40 arcsec circular ap. mag. | ||||
| J_M_50 | float | mag | J-band circular aperture magnitude (50 arcsec radius) | |||
| J_MSIG_50 | float | mag | error in J-band circular aperture magnitude (50 arcsec radius) | |||
| J_FLG_50 | int | J confusion flag for 50 arcsec circular ap. mag. | ||||
| J_M_60 | float | mag | J-band circular aperture magnitude (60 arcsec radius) | |||
| J_MSIG_60 | float | mag | error in J-band circular aperture magnitude (60 arcsec radius) | |||
| J_FLG_60 | int | J confusion flag for 60 arcsec circular ap. mag. | ||||
| J_M_70 | float | mag | J-band circular aperture magnitude (70 arcsec radius) | |||
| J_MSIG_70 | float | mag | error in J-band circular aperture magnitude (70 arcsec radius) | |||
| J_FLG_70 | int | J confusion flag for 70 arcsec circular ap. mag. | ||||
| H_M_5 | float | mag | H-band circular aperture magnitude (5 arcsec radius) | |||
| H_MSIG_5 | float | mag | error in H-band circular aperture magnitude (5 arcsec radius) | |||
| H_FLG_5 | int | H confusion flag for 5 arcsec circular ap. mag. | ||||
| H_M_7 | float | mag | H-band circular aperture magnitude (7 arcsec radius) | |||
| H_MSIG_7 | float | mag | error in H-band circular aperture magnitude (7 arcsec radius) | |||
| H_FLG_7 | int | H confusion flag for 7 arcsec circular ap. mag. | ||||
| H_M_10 | float | mag | H-band circular aperture magnitude (10 arcsec radius) | |||
| H_MSIG_10 | float | mag | error in H-band circular aperture magnitude (10 arcsec radius) | |||
| H_FLG_10 | int | H confusion flag for 10 arcsec circular ap. mag. | ||||
| H_M_15 | float | mag | H-band circular aperture magnitude (15 arcsec radius) | |||
| H_MSIG_15 | float | mag | error in H-band circular aperture magnitude (15 arcsec radius) | |||
| H_FLG_15 | int | H confusion flag for 15 arcsec circular ap. mag. | ||||
| H_M_20 | float | mag | H-band circular aperture magnitude (20 arcsec radius) | |||
| H_MSIG_20 | float | mag | error in H-band circular aperture magnitude (20 arcsec radius) | |||
| H_FLG_20 | int | H confusion flag for 20 arcsec circular ap. mag. | ||||
| H_M_25 | float | mag | H-band circular aperture magnitude (25 arcsec radius) | |||
| H_MSIG_25 | float | mag | error in H-band circular aperture magnitude (25 arcsec radius) | |||
| H_FLG_25 | int | H confusion flag for 25 arcsec circular ap. mag. | ||||
| H_M_30 | float | mag | H-band circular aperture magnitude (30 arcsec radius) | |||
| H_MSIG_30 | float | mag | error in H-band circular aperture magnitude (30 arcsec radius) | |||
| H_FLG_30 | int | H confusion flag for 30 arcsec circular ap. mag. | ||||
| H_M_40 | float | mag | H-band circular aperture magnitude (40 arcsec radius) | |||
| H_MSIG_40 | float | mag | error in H-band circular aperture magnitude (40 arcsec radius) | |||
| H_FLG_40 | int | H confusion flag for 40 arcsec circular ap. mag. | ||||
| H_M_50 | float | mag | H-band circular aperture magnitude (50 arcsec radius) | |||
| H_MSIG_50 | float | mag | error in H-band circular aperture magnitude (50 arcsec radius) | |||
| H_FLG_50 | int | H confusion flag for 50 arcsec circular ap. mag. | ||||
| H_M_60 | float | mag | H-band circular aperture magnitude (60 arcsec radius) | |||
| H_MSIG_60 | float | mag | error in H-band circular aperture magnitude (60 arcsec radius) | |||
| H_FLG_60 | int | H confusion flag for 60 arcsec circular ap. mag. | ||||
| H_M_70 | float | mag | H-band circular aperture magnitude (70 arcsec radius) | |||
| H_MSIG_70 | float | mag | error in H-band circular aperture magnitude (70 arcsec radius) | |||
| H_FLG_70 | int | H confusion flag for 70 arcsec circular ap. mag. | ||||
| K_M_5 | float | mag | K-band circular aperture magnitude (5 arcsec radius) | |||
| K_MSIG_5 | float | mag | error in K-band circular aperture magnitude (5 arcsec radius) | |||
| K_FLG_5 | int | K confusion flag for 5 arcsec circular ap. mag. | ||||
| K_M_7 | float | mag | K-band circular aperture magnitude (7 arcsec radius) | |||
| K_MSIG_7 | float | mag | error in K-band circular aperture magnitude (7 arcsec radius) | |||
| K_FLG_7 | int | K confusion flag for 7 arcsec circular ap. mag. | ||||
| K_M_10 | float | mag | K-band circular aperture magnitude (10 arcsec radius) | |||
| K_MSIG_10 | float | mag | error in K-band circular aperture magnitude (10 arcsec radius) | |||
| K_FLG_10 | int | K confusion flag for 10 arcsec circular ap. mag. | ||||
| K_M_15 | float | mag | K-band circular aperture magnitude (15 arcsec radius) | |||
| K_MSIG_15 | float | mag | error in K-band circular aperture magnitude (15 arcsec radius) | |||
| K_FLG_15 | int | K confusion flag for 15 arcsec circular ap. mag. | ||||
| K_M_20 | float | mag | K-band circular aperture magnitude (20 arcsec radius) | |||
| K_MSIG_20 | float | mag | error in K-band circular aperture magnitude (20 arcsec radius) | |||
| K_FLG_20 | int | K confusion flag for 20 arcsec circular ap. mag. | ||||
| K_M_25 | float | mag | K-band circular aperture magnitude (25 arcsec radius) | |||
| K_MSIG_25 | float | mag | error in K-band circular aperture magnitude (25 arcsec radius) | |||
| K_FLG_25 | int | K confusion flag for 25 arcsec circular ap. mag. | ||||
| K_M_30 | float | mag | K-band circular aperture magnitude (30 arcsec radius) | |||
| K_MSIG_30 | float | mag | error in K-band circular aperture magnitude (30 arcsec radius) | |||
| K_FLG_30 | int | K confusion flag for 30 arcsec circular ap. mag. | ||||
| K_M_40 | float | mag | K-band circular aperture magnitude (40 arcsec radius) | |||
| K_MSIG_40 | float | mag | error in K-band circular aperture magnitude (40 arcsec radius) | |||
| K_FLG_40 | int | K confusion flag for 40 arcsec circular ap. mag. | ||||
| K_M_50 | float | mag | K-band circular aperture magnitude (50 arcsec radius) | |||
| K_MSIG_50 | float | mag | error in K-band circular aperture magnitude (50 arcsec radius) | |||
| K_FLG_50 | int | K confusion flag for 50 arcsec circular ap. mag. | ||||
| K_M_60 | float | mag | K-band circular aperture magnitude (60 arcsec radius) | |||
| K_MSIG_60 | float | mag | error in K-band circular aperture magnitude (60 arcsec radius) | |||
| K_FLG_60 | int | K confusion flag for 60 arcsec circular ap. mag. | ||||
| K_M_70 | float | mag | K-band circular aperture magnitude (70 arcsec radius) | |||
| K_MSIG_70 | float | mag | error in K-band circular aperture magnitude (70 arcsec radius) | |||
| K_FLG_70 | int | K confusion flag for 70 arcsec circular ap. mag. |
SDSS objects that match to USNO-B objects have their match parameters stored her
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| OBJID | long | unique id, points to photoObj | ||||
| RA | double | deg | J2000 right ascension in USNO-B1.0 | |||
| DEC | double | deg | J2000 declination in USNO-B1.0 | |||
| RAERR | double | arcsec | error in R.A. | |||
| DECERR | double | arcsec | error in Dec | |||
| MEANEPOCH | double | years | mean epoch of RA/Dec | |||
| MURA | float | mas/yr | proper motion in RA | |||
| MUDEC | float | mas/yr | proper motion in Dec | |||
| PROPERMOTION | float | 0.01 arcsec/yr | total proper motion | |||
| ANGLE | float | deg | position angle of proper motion (East of North) | |||
| MURAERR | float | mas/yr | error in proper motion in RA | |||
| MUDECERR | float | mas/yr | error in proper motion in Dec | |||
| MUPROB | float | probability of proper motion | ||||
| MUFLAG | int | proper motion flag (0 no, 1 yes) | ||||
| SFITRA | float | mas | sigma of individual observations around best fit motion in RA | |||
| SFITDEC | float | mas | sigma of individual observations around best fit motion in RA | |||
| NFITPT | int | number of observations used in the fit | ||||
| MAG_B1 | float | mag | ||||
| MAG_R1 | float | mag | ||||
| MAG_B2 | float | mag | ||||
| MAG_R2 | float | mag | ||||
| MAG_I2 | float | mag | ||||
| FLDID_B1 | int | field id in first blue survey | ||||
| FLDID_R1 | int | field id in first red survey | ||||
| FLDID_B2 | int | field id in second blue survey | ||||
| FLDID_R2 | int | field id in second red survey | ||||
| FLDID_I2 | int | field id in N survey | ||||
| SG_B1 | int | star/galaxy separation flag in first blue survey (values of 0 to 3 are probably stellar, values of 8 to 11 are probably non-stellar) | ||||
| SG_R1 | int | star/galaxy separation flag in first red survey (values of 0 to 3 are probably stellar, values of 8 to 11 are probably non-stellar) | ||||
| SG_B2 | int | star/galaxy separation flag in second blue survey (values of 0 to 3 are probably stellar, values of 8 to 11 are probably non-stellar) | ||||
| SG_R2 | int | star/galaxy separation flag in second red survey (values of 0 to 3 are probably stellar, values of 8 to 11 are probably non-stellar) | ||||
| SG_I2 | int | star/galaxy separation flag in N survey (values of 0 to 3 are probably stellar, values of 8 to 11 are probably non-stellar) | ||||
| FLDEPOCH_B1 | float | epoch of observation in first blue survey | ||||
| FLDEPOCH_R1 | float | epoch of observation in first red survey | ||||
| FLDEPOCH_B2 | float | epoch of observation in second blue survey | ||||
| FLDEPOCH_R2 | float | epoch of observation in second red survey | ||||
| FLDEPOCH_I2 | float | epoch of observation in N survey |
Tracks the versioning history of the databas
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| event | string | The event that happened | ||||
| previous | string | Version before the patch | ||||
| checksum | string | Checksum before the patch | ||||
| version | string | Version after the patch | ||||
| description | string | Summary of changes | ||||
| text | string | Details of changes in HTML form | ||||
| who | string | Person(s) responsible | ||||
| when | string | When it happened |
Table to organize objects into declination zone
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| zoneID | int | id counts from -90 degrees == 0 | ||||
| ra | double | deg | ra of object | |||
| dec | double | deg | declination of object | |||
| objID | long | object ID | ||||
| type | int | object type (star, galaxy) | ||||
| mode | int | mode is primary, secondary, family, outside | ||||
| cx | double | Cartesian x of the object | ||||
| cy | double | Cartesian y of the object | ||||
| cz | double | Cartesian z of the object | ||||
| native | int | true if obj is local, false if from the destination dataset |
Full list of all detections, with associated 'thing' assignment
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| thingId | long | thing ID number | ||||
| objId | long | object ID number (from run, camcol, field, id, rerun) | ||||
| loadVersion | int | Load Version |
Emission line kinematics results for BOSS galaxies using GANDAL
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| specObjID | long | Unique ID | ||||
| plate | int | Plate number | ||||
| fiberID | int | Fiber ID | ||||
| mjd | int | days | MJD of observation | |||
| ra | double | deg | Right ascension of fiber, J2000 | |||
| dec | double | deg | Declination of fiber, J2000 | |||
| z | float | Redshift used (corresponds to z_noqso in specObjAll) | ||||
| zErr | float | Error in z (corresponds to zErr_noqso in specObjAll) | ||||
| zNum | int | Index of chi^2 minimum corresponding to z_noqso | ||||
| velStars | float | km/s | stellar velocity | |||
| redshift | float | GANDALF-corrected redshift | ||||
| sigmaStars | float | km/s | Stellar velocity dispersion | |||
| sigmaStarsErr | float | km/s | Error on measurement of stellar velocity dispersion | |||
| chisq | float | chi-squared of best-fit template | ||||
| bpt | string | Classification from Kauffmann et al. (2003), Kewley et al. (2001) and Schawinski et al. (2007) for objects with the emission lines Hβ, [OIII], Hα, [NII] available with A/N > 1.5. Possible values: "BLANK" (if emission lines not available), "Star Forming", "Seyfert", "LINER", "Seyfert/LINER", "Composite" | ||||
| ebmv | float | mag | E(B-V) for internal reddening estimated from emission lines | |||
| ebmv_err | float | mag | Error in E(B-V)for internal reddening estimated from emission lines | |||
| Error_Warning | int | Set to 1 if error calculation failed (errors all set to zero in that case); otherwise, set to 0 | ||||
| V_HeII_3203 | float | km/s | Velocity of emission line HeII 3203 | |||
| V_HeII_3203_Err | float | km/s | Error in velocity of emission line HeII 3203 | |||
| Sigma_HeII_3203 | float | km/s | Velocity dispersion of emission line HeII 3203 | |||
| Sigma_HeII_3203_Err | float | km/s | Error in velocity dispersion of emission line HeII 3203 | |||
| Amplitude_HeII_3203 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line HeII 3203 | |||
| Amplitude_HeII_3203_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line HeII 3203 | |||
| Flux_HeII_3203 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line HeII 3203 | |||
| Flux_HeII_3203_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line HeII 3203 | |||
| EW_HeII_3203 | float | Angstroms | Equivalent width of emission line HeII 3203 | |||
| EW_HeII_3203_Err | float | Angstroms | Error in equivalent width of emission line HeII 3203 | |||
| Flux_Cont_HeII_3203 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line HeII 3203 | |||
| Flux_Cont_HeII_3203_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line HeII 3203 | |||
| Fit_Warning_HeII_3203 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| AoN_HeII_3203 | float | km/s | Amplitude-over-noise of emission line HeII 3203 | |||
| V_NeV_3345 | float | km/s | Velocity of emission line [NeV] 3345 | |||
| V_NeV_3345_Err | float | km/s | Error in velocity of emission line [NeV] 3345 | |||
| Sigma_NeV_3345 | float | km/s | Velocity dispersion of emission line [NeV] 3345 | |||
| Sigma_NeV_3345_Err | float | km/s | Error in velocity dispersion of emission line [NeV] 3345 | |||
| Amplitude_NeV_3345 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line [NeV] 3345 | |||
| Amplitude_NeV_3345_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line [NeV] 3345 | |||
| Flux_NeV_3345 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line [NeV] 3345 | |||
| Flux_NeV_3345_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line [NeV] 3345 | |||
| EW_NeV_3345 | float | Angstroms | Equivalent width of emission line [NeV] 3345 | |||
| EW_NeV_3345_Err | float | Angstroms | Error in equivalent width of emission line [NeV] 3345 | |||
| Flux_Cont_NeV_3345 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line [NeV] 3345 | |||
| Flux_Cont_NeV_3345_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line [NeV] 3345 | |||
| Fit_Warning_NeV_3345 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| AoN_NeV_3345 | float | km/s | Amplitude-over-noise of emission line [NeV] 3345 | |||
| V_NeV_3425 | float | km/s | Velocity of emission line [NeV] 3425 | |||
| V_NeV_3425_Err | float | km/s | Error in velocity of emission line [NeV] 3425 | |||
| Sigma_NeV_3425 | float | km/s | Velocity dispersion of emission line [NeV] 3425 | |||
| Sigma_NeV_3425_Err | float | km/s | Error in velocity dispersion of emission line [NeV] 3425 | |||
| Amplitude_NeV_3425 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line [NeV] 3425 | |||
| Amplitude_NeV_3425_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line [NeV] 3425 | |||
| Flux_NeV_3425 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line [NeV] 3425 | |||
| Flux_NeV_3425_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line [NeV] 3425 | |||
| EW_NeV_3425 | float | Angstroms | Equivalent width of emission line [NeV] 3425 | |||
| EW_NeV_3425_Err | float | Angstroms | Error in equivalent width of emission line [NeV] 3425 | |||
| Flux_Cont_NeV_3425 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line [NeV] 3425 | |||
| Flux_Cont_NeV_3425_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line [NeV] 3425 | |||
| Fit_Warning_NeV_3425 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| AoN_NeV_3425 | float | km/s | Amplitude-over-noise of emission line [NeV] 3425 | |||
| V_OII_3726 | float | km/s | Velocity of emission line [OII] 3726 | |||
| V_OII_3726_Err | float | km/s | Error in velocity of emission line [OII] 3726 | |||
| Sigma_OII_3726 | float | km/s | Velocity dispersion of emission line [OII] 3726 | |||
| Sigma_OII_3726_Err | float | km/s | Error in velocity dispersion of emission line [OII] 3726 | |||
| Amplitude_OII_3726 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line [OII] 3726 | |||
| Amplitude_OII_3726_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line [OII] 3726 | |||
| Flux_OII_3726 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line [OII] 3726 | |||
| Flux_OII_3726_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line [OII] 3726 | |||
| EW_OII_3726 | float | Angstroms | Equivalent width of emission line [OII] 3726 | |||
| EW_OII_3726_Err | float | Angstroms | Error in equivalent width of emission line [OII] 3726 | |||
| Flux_Cont_OII_3726 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line [OII] 3726 | |||
| Flux_Cont_OII_3726_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line [OII] 3726 | |||
| Fit_Warning_OII_3726 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| AoN_OII_3726 | float | km/s | Amplitude-over-noise of emission line [OII] 3726 | |||
| V_OII_3728 | float | km/s | Velocity of emission line [OII] 3728 | |||
| V_OII_3728_Err | float | km/s | Error in velocity of emission line [OII] 3728 | |||
| Sigma_OII_3728 | float | km/s | Velocity dispersion of emission line [OII] 3728 | |||
| Sigma_OII_3728_Err | float | km/s | Error in velocity dispersion of emission line [OII] 3728 | |||
| Amplitude_OII_3728 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line [OII] 3728 | |||
| Amplitude_OII_3728_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line [OII] 3728 | |||
| Flux_OII_3728 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line [OII] 3728 | |||
| Flux_OII_3728_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line [OII] 3728 | |||
| EW_OII_3728 | float | Angstroms | Equivalent width of emission line [OII] 3728 | |||
| EW_OII_3728_Err | float | Angstroms | Error in equivalent width of emission line [OII] 3728 | |||
| Flux_Cont_OII_3728 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line [OII] 3728 | |||
| Flux_Cont_OII_3728_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line [OII] 3728 | |||
| Fit_Warning_OII_3728 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| AoN_OII_3728 | float | km/s | Amplitude-over-noise of emission line [OII] 3728 | |||
| V_NeIII_3868 | float | km/s | Velocity of emission line [NeIII] 3868 | |||
| V_NeIII_3868_Err | float | km/s | Error in velocity of emission line [NeIII] 3868 | |||
| Sigma_NeIII_3868 | float | km/s | Velocity dispersion of emission line [NeIII] 3868 | |||
| Sigma_NeIII_3868_Err | float | km/s | Error in velocity dispersion of emission line [NeIII] 3868 | |||
| Amplitude_NeIII_3868 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line [NeIII] 3868 | |||
| Amplitude_NeIII_3868_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line [NeIII] 3868 | |||
| Flux_NeIII_3868 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line [NeIII] 3868 | |||
| Flux_NeIII_3868_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line [NeIII] 3868 | |||
| EW_NeIII_3868 | float | Angstroms | Equivalent width of emission line [NeIII] 3868 | |||
| EW_NeIII_3868_Err | float | Angstroms | Error in equivalent width of emission line [NeIII] 3868 | |||
| Flux_Cont_NeIII_3868 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line [NeIII] 3868 | |||
| Flux_Cont_NeIII_3868_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line [NeIII] 3868 | |||
| Fit_Warning_NeIII_3868 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| AoN_NeIII_3868 | float | km/s | Amplitude-over-noise of emission line [NeIII] 3868 | |||
| V_NeIII_3967 | float | km/s | Velocity of emission line [NeIII] 3967 | |||
| V_NeIII_3967_Err | float | km/s | Error in velocity of emission line [NeIII] 3967 | |||
| Sigma_NeIII_3967 | float | km/s | Velocity dispersion of emission line [NeIII] 3967 | |||
| Sigma_NeIII_3967_Err | float | km/s | Error in velocity dispersion of emission line [NeIII] 3967 | |||
| Amplitude_NeIII_3967 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line [NeIII] 3967 | |||
| Amplitude_NeIII_3967_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line [NeIII] 3967 | |||
| Flux_NeIII_3967 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line [NeIII] 3967 | |||
| Flux_NeIII_3967_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line [NeIII] 3967 | |||
| EW_NeIII_3967 | float | Angstroms | Equivalent width of emission line [NeIII] 3967 | |||
| EW_NeIII_3967_Err | float | Angstroms | Error in equivalent width of emission line [NeIII] 3967 | |||
| Flux_Cont_NeIII_3967 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line [NeIII] 3967 | |||
| Flux_Cont_NeIII_3967_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line [NeIII] 3967 | |||
| Fit_Warning_NeIII_3967 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| AoN_NeIII_3967 | float | km/s | Amplitude-over-noise of emission line [NeIII] 3967 | |||
| V_H5_3889 | float | km/s | Velocity of emission line H5 3889 | |||
| V_H5_3889_Err | float | km/s | Error in velocity of emission line H5 3889 | |||
| Sigma_H5_3889 | float | km/s | Velocity dispersion of emission line H5 3889 | |||
| Sigma_H5_3889_Err | float | km/s | Error in velocity dispersion of emission line H5 3889 | |||
| Amplitude_H5_3889 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line H5 3889 | |||
| Amplitude_H5_3889_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line H5 3889 | |||
| Flux_H5_3889 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line H5 3889 | |||
| Flux_H5_3889_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line H5 3889 | |||
| EW_H5_3889 | float | Angstroms | Equivalent width of emission line H5 3889 | |||
| EW_H5_3889_Err | float | Angstroms | Error in equivalent width of emission line H5 3889 | |||
| Flux_Cont_H5_3889 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line H5 3889 | |||
| Flux_Cont_H5_3889_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line H5 3889 | |||
| Fit_Warning_H5_3889 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| AoN_H5_3889 | float | km/s | Amplitude-over-noise of emission line H5 3889 | |||
| V_He_3970 | float | km/s | Velocity of emission line He 3970 | |||
| V_He_3970_Err | float | km/s | Error in velocity of emission line He 3970 | |||
| Sigma_He_3970 | float | km/s | Velocity dispersion of emission line He 3970 | |||
| Sigma_He_3970_Err | float | km/s | Error in velocity dispersion of emission line He 3970 | |||
| Amplitude_He_3970 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line He 3970 | |||
| Amplitude_He_3970_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line He 3970 | |||
| Flux_He_3970 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line He 3970 | |||
| Flux_He_3970_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line He 3970 | |||
| EW_He_3970 | float | Angstroms | Equivalent width of emission line He 3970 | |||
| EW_He_3970_Err | float | Angstroms | Error in equivalent width of emission line He 3970 | |||
| Flux_Cont_He_3970 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line He 3970 | |||
| Flux_Cont_He_3970_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line He 3970 | |||
| Fit_Warning_He_3970 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| AoN_He_3970 | float | km/s | Amplitude-over-noise of emission line He 3970 | |||
| V_Hd_4101 | float | km/s | Velocity of emission line Hd 4101 | |||
| V_Hd_4101_Err | float | km/s | Error in velocity of emission line Hd 4101 | |||
| Sigma_Hd_4101 | float | km/s | Velocity dispersion of emission line Hd 4101 | |||
| Sigma_Hd_4101_Err | float | km/s | Error in velocity dispersion of emission line Hd 4101 | |||
| Amplitude_Hd_4101 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line Hd 4101 | |||
| Amplitude_Hd_4101_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line Hd 4101 | |||
| Flux_Hd_4101 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line Hd 4101 | |||
| Flux_Hd_4101_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line Hd 4101 | |||
| EW_Hd_4101 | float | Angstroms | Equivalent width of emission line Hd 4101 | |||
| EW_Hd_4101_Err | float | Angstroms | Error in equivalent width of emission line Hd 4101 | |||
| Flux_Cont_Hd_4101 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line Hd 4101 | |||
| Flux_Cont_Hd_4101_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line Hd 4101 | |||
| Fit_Warning_Hd_4101 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| AoN_Hd_4101 | float | km/s | Amplitude-over-noise of emission line Hd 4101 | |||
| V_Hg_4340 | float | km/s | Velocity of emission line Hg 4340 | |||
| V_Hg_4340_Err | float | km/s | Error in velocity of emission line Hg 4340 | |||
| Sigma_Hg_4340 | float | km/s | Velocity dispersion of emission line Hg 4340 | |||
| Sigma_Hg_4340_Err | float | km/s | Error in velocity dispersion of emission line Hg 4340 | |||
| Amplitude_Hg_4340 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line Hg 4340 | |||
| Amplitude_Hg_4340_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line Hg 4340 | |||
| Flux_Hg_4340 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line Hg 4340 | |||
| Flux_Hg_4340_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line Hg 4340 | |||
| EW_Hg_4340 | float | Angstroms | Equivalent width of emission line Hg 4340 | |||
| EW_Hg_4340_Err | float | Angstroms | Error in equivalent width of emission line Hg 4340 | |||
| Flux_Cont_Hg_4340 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line Hg 4340 | |||
| Flux_Cont_Hg_4340_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line Hg 4340 | |||
| Fit_Warning_Hg_4340 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| AoN_Hg_4340 | float | km/s | Amplitude-over-noise of emission line Hg 4340 | |||
| V_OIII_4363 | float | km/s | Velocity of emission line [OIII] 4363 | |||
| V_OIII_4363_Err | float | km/s | Error in velocity of emission line [OIII] 4363 | |||
| Sigma_OIII_4363 | float | km/s | Velocity dispersion of emission line [OIII] 4363 | |||
| Sigma_OIII_4363_Err | float | km/s | Error in velocity dispersion of emission line [OIII] 4363 | |||
| Amplitude_OIII_4363 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line [OIII] 4363 | |||
| Amplitude_OIII_4363_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line [OIII] 4363 | |||
| Flux_OIII_4363 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line [OIII] 4363 | |||
| Flux_OIII_4363_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line [OIII] 4363 | |||
| EW_OIII_4363 | float | Angstroms | Equivalent width of emission line [OIII] 4363 | |||
| EW_OIII_4363_Err | float | Angstroms | Error in equivalent width of emission line [OIII] 4363 | |||
| Flux_Cont_OIII_4363 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line [OIII] 4363 | |||
| Flux_Cont_OIII_4363_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line [OIII] 4363 | |||
| Fit_Warning_OIII_4363 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| AoN_OIII_4363 | float | km/s | Amplitude-over-noise of emission line [OIII] 4363 | |||
| V_HeII_4685 | float | km/s | Velocity of emission line HeII 4685 | |||
| V_HeII_4685_Err | float | km/s | Error in velocity of emission line HeII 4685 | |||
| Sigma_HeII_4685 | float | km/s | Velocity dispersion of emission line HeII 4685 | |||
| Sigma_HeII_4685_Err | float | km/s | Error in velocity dispersion of emission line HeII 4685 | |||
| Amplitude_HeII_4685 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line HeII 4685 | |||
| Amplitude_HeII_4685_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line HeII 4685 | |||
| Flux_HeII_4685 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line HeII 4685 | |||
| Flux_HeII_4685_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line HeII 4685 | |||
| EW_HeII_4685 | float | Angstroms | Equivalent width of emission line HeII 4685 | |||
| EW_HeII_4685_Err | float | Angstroms | Error in equivalent width of emission line HeII 4685 | |||
| Flux_Cont_HeII_4685 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line HeII 4685 | |||
| Flux_Cont_HeII_4685_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line HeII 4685 | |||
| Fit_Warning_HeII_4685 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| AoN_HeII_4685 | float | km/s | Amplitude-over-noise of emission line HeII 4685 | |||
| V_ArIV_4711 | float | km/s | Velocity of emission line [ArIV] 4711 | |||
| V_ArIV_4711_Err | float | km/s | Error in velocity of emission line [ArIV] 4711 | |||
| Sigma_ArIV_4711 | float | km/s | Velocity dispersion of emission line [ArIV] 4711 | |||
| Sigma_ArIV_4711_Err | float | km/s | Error in velocity dispersion of emission line [ArIV] 4711 | |||
| Amplitude_ArIV_4711 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line [ArIV] 4711 | |||
| Amplitude_ArIV_4711_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line [ArIV] 4711 | |||
| Flux_ArIV_4711 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line [ArIV] 4711 | |||
| Flux_ArIV_4711_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line [ArIV] 4711 | |||
| EW_ArIV_4711 | float | Angstroms | Equivalent width of emission line [ArIV] 4711 | |||
| EW_ArIV_4711_Err | float | Angstroms | Error in equivalent width of emission line [ArIV] 4711 | |||
| Flux_Cont_ArIV_4711 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line [ArIV] 4711 | |||
| Flux_Cont_ArIV_4711_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line [ArIV] 4711 | |||
| Fit_Warning_ArIV_4711 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| AoN_ArIV_4711 | float | km/s | Amplitude-over-noise of emission line [ArIV] 4711 | |||
| V_ArIV_4740 | float | km/s | Velocity of emission line [ArIV] 4740 | |||
| V_ArIV_4740_Err | float | km/s | Error in velocity of emission line [ArIV] 4740 | |||
| Sigma_ArIV_4740 | float | km/s | Velocity dispersion of emission line [ArIV] 4740 | |||
| Sigma_ArIV_4740_Err | float | km/s | Error in velocity dispersion of emission line [ArIV] 4740 | |||
| Amplitude_ArIV_4740 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line [ArIV] 4740 | |||
| Amplitude_ArIV_4740_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line [ArIV] 4740 | |||
| Flux_ArIV_4740 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line [ArIV] 4740 | |||
| Flux_ArIV_4740_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line [ArIV] 4740 | |||
| EW_ArIV_4740 | float | Angstroms | Equivalent width of emission line [ArIV] 4740 | |||
| EW_ArIV_4740_Err | float | Angstroms | Error in equivalent width of emission line [ArIV] 4740 | |||
| Flux_Cont_ArIV_4740 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line [ArIV] 4740 | |||
| Flux_Cont_ArIV_4740_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line [ArIV] 4740 | |||
| Fit_Warning_ArIV_4740 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| AoN_ArIV_4740 | float | km/s | Amplitude-over-noise of emission line [ArIV] 4740 | |||
| V_Hb_4861 | float | km/s | Velocity of emission line Hb 4861 | |||
| V_Hb_4861_Err | float | km/s | Error in velocity of emission line Hb 4861 | |||
| Sigma_Hb_4861 | float | km/s | Velocity dispersion of emission line Hb 4861 | |||
| Sigma_Hb_4861_Err | float | km/s | Error in velocity dispersion of emission line Hb 4861 | |||
| Amplitude_Hb_4861 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line Hb 4861 | |||
| Amplitude_Hb_4861_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line Hb 4861 | |||
| Flux_Hb_4861 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line Hb 4861 | |||
| Flux_Hb_4861_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line Hb 4861 | |||
| EW_Hb_4861 | float | Angstroms | Equivalent width of emission line Hb 4861 | |||
| EW_Hb_4861_Err | float | Angstroms | Error in equivalent width of emission line Hb 4861 | |||
| Flux_Cont_Hb_4861 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line Hb 4861 | |||
| Flux_Cont_Hb_4861_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line Hb 4861 | |||
| Fit_Warning_Hb_4861 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| AoN_Hb_4861 | float | km/s | Amplitude-over-noise of emission line Hb 4861 | |||
| V_OIII_4958 | float | km/s | Velocity of emission line [OIII] 4958 | |||
| V_OIII_4958_Err | float | km/s | Error in velocity of emission line [OIII] 4958 | |||
| Sigma_OIII_4958 | float | km/s | Velocity dispersion of emission line [OIII] 4958 | |||
| Sigma_OIII_4958_Err | float | km/s | Error in velocity dispersion of emission line [OIII] 4958 | |||
| Amplitude_OIII_4958 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line [OIII] 4958 | |||
| Amplitude_OIII_4958_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line [OIII] 4958 | |||
| Flux_OIII_4958 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line [OIII] 4958 | |||
| Flux_OIII_4958_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line [OIII] 4958 | |||
| EW_OIII_4958 | float | Angstroms | Equivalent width of emission line [OIII] 4958 | |||
| EW_OIII_4958_Err | float | Angstroms | Error in equivalent width of emission line [OIII] 4958 | |||
| Flux_Cont_OIII_4958 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line [OIII] 4958 | |||
| Flux_Cont_OIII_4958_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line [OIII] 4958 | |||
| Fit_Warning_OIII_4958 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| V_OIII_5006 | float | km/s | Velocity of emission line [OIII] 5006 | |||
| V_OIII_5006_Err | float | km/s | Error in velocity of emission line [OIII] 5006 | |||
| Sigma_OIII_5006 | float | km/s | Velocity dispersion of emission line [OIII] 5006 | |||
| Sigma_OIII_5006_Err | float | km/s | Error in velocity dispersion of emission line [OIII] 5006 | |||
| Amplitude_OIII_5006 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line [OIII] 5006 | |||
| Amplitude_OIII_5006_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line [OIII] 5006 | |||
| Flux_OIII_5006 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line [OIII] 5006 | |||
| Flux_OIII_5006_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line [OIII] 5006 | |||
| EW_OIII_5006 | float | Angstroms | Equivalent width of emission line [OIII] 5006 | |||
| EW_OIII_5006_Err | float | Angstroms | Error in equivalent width of emission line [OIII] 5006 | |||
| Flux_Cont_OIII_5006 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line [OIII] 5006 | |||
| Flux_Cont_OIII_5006_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line [OIII] 5006 | |||
| Fit_Warning_OIII_5006 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| AoN_OIII_5006 | float | km/s | Amplitude-over-noise of emission line [OIII] 5006 | |||
| V_NI_5197 | float | km/s | Velocity of emission line [NI] 5197 | |||
| V_NI_5197_Err | float | km/s | Error in velocity of emission line [NI] 5197 | |||
| Sigma_NI_5197 | float | km/s | Velocity dispersion of emission line [NI] 5197 | |||
| Sigma_NI_5197_Err | float | km/s | Error in velocity dispersion of emission line [NI] 5197 | |||
| Amplitude_NI_5197 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line [NI] 5197 | |||
| Amplitude_NI_5197_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line [NI] 5197 | |||
| Flux_NI_5197 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line [NI] 5197 | |||
| Flux_NI_5197_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line [NI] 5197 | |||
| EW_NI_5197 | float | Angstroms | Equivalent width of emission line [NI] 5197 | |||
| EW_NI_5197_Err | float | Angstroms | Error in equivalent width of emission line [NI] 5197 | |||
| Flux_Cont_NI_5197 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line [NI] 5197 | |||
| Flux_Cont_NI_5197_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line [NI] 5197 | |||
| Fit_Warning_NI_5197 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| AoN_NI_5197 | float | km/s | Amplitude-over-noise of emission line [NI] 5197 | |||
| V_NI_5200 | float | km/s | Velocity of emission line [NI] 5200 | |||
| V_NI_5200_Err | float | km/s | Error in velocity of emission line [NI] 5200 | |||
| Sigma_NI_5200 | float | km/s | Velocity dispersion of emission line [NI] 5200 | |||
| Sigma_NI_5200_Err | float | km/s | Error in velocity dispersion of emission line [NI] 5200 | |||
| Amplitude_NI_5200 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line [NI] 5200 | |||
| Amplitude_NI_5200_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line [NI] 5200 | |||
| Flux_NI_5200 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line [NI] 5200 | |||
| Flux_NI_5200_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line [NI] 5200 | |||
| EW_NI_5200 | float | Angstroms | Equivalent width of emission line [NI] 5200 | |||
| EW_NI_5200_Err | float | Angstroms | Error in equivalent width of emission line [NI] 5200 | |||
| Flux_Cont_NI_5200 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line [NI] 5200 | |||
| Flux_Cont_NI_5200_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line [NI] 5200 | |||
| Fit_Warning_NI_5200 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| AoN_NI_5200 | float | km/s | Amplitude-over-noise of emission line [NI] 5200 | |||
| V_HeI_5875 | float | km/s | Velocity of emission line HeI 5875 | |||
| V_HeI_5875_Err | float | km/s | Error in velocity of emission line HeI 5875 | |||
| Sigma_HeI_5875 | float | km/s | Velocity dispersion of emission line HeI 5875 | |||
| Sigma_HeI_5875_Err | float | km/s | Error in velocity dispersion of emission line HeI 5875 | |||
| Amplitude_HeI_5875 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line HeI 5875 | |||
| Amplitude_HeI_5875_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line HeI 5875 | |||
| Flux_HeI_5875 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line HeI 5875 | |||
| Flux_HeI_5875_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line HeI 5875 | |||
| EW_HeI_5875 | float | Angstroms | Equivalent width of emission line HeI 5875 | |||
| EW_HeI_5875_Err | float | Angstroms | Error in equivalent width of emission line HeI 5875 | |||
| Flux_Cont_HeI_5875 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line HeI 5875 | |||
| Flux_Cont_HeI_5875_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line HeI 5875 | |||
| Fit_Warning_HeI_5875 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| AoN_HeI_5875 | float | km/s | Amplitude-over-noise of emission line HeI 5875 | |||
| V_OI_6300 | float | km/s | Velocity of emission line [OI] 6300 | |||
| V_OI_6300_Err | float | km/s | Error in velocity of emission line [OI] 6300 | |||
| Sigma_OI_6300 | float | km/s | Velocity dispersion of emission line [OI] 6300 | |||
| Sigma_OI_6300_Err | float | km/s | Error in velocity dispersion of emission line [OI] 6300 | |||
| Amplitude_OI_6300 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line [OI] 6300 | |||
| Amplitude_OI_6300_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line [OI] 6300 | |||
| Flux_OI_6300 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line [OI] 6300 | |||
| Flux_OI_6300_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line [OI] 6300 | |||
| EW_OI_6300 | float | Angstroms | Equivalent width of emission line [OI] 6300 | |||
| EW_OI_6300_Err | float | Angstroms | Error in equivalent width of emission line [OI] 6300 | |||
| Flux_Cont_OI_6300 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line [OI] 6300 | |||
| Flux_Cont_OI_6300_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line [OI] 6300 | |||
| Fit_Warning_OI_6300 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| AoN_OI_6300 | float | km/s | Amplitude-over-noise of emission line [OI] 6300 | |||
| V_OI_6363 | float | km/s | Velocity of emission line [OI] 6363 | |||
| V_OI_6363_Err | float | km/s | Error in velocity of emission line [OI] 6363 | |||
| Sigma_OI_6363 | float | km/s | Velocity dispersion of emission line [OI] 6363 | |||
| Sigma_OI_6363_Err | float | km/s | Error in velocity dispersion of emission line [OI] 6363 | |||
| Amplitude_OI_6363 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line [OI] 6363 | |||
| Amplitude_OI_6363_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line [OI] 6363 | |||
| Flux_OI_6363 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line [OI] 6363 | |||
| Flux_OI_6363_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line [OI] 6363 | |||
| EW_OI_6363 | float | Angstroms | Equivalent width of emission line [OI] 6363 | |||
| EW_OI_6363_Err | float | Angstroms | Error in equivalent width of emission line [OI] 6363 | |||
| Flux_Cont_OI_6363 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line [OI] 6363 | |||
| Flux_Cont_OI_6363_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line [OI] 6363 | |||
| Fit_Warning_OI_6363 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| AoN_OI_6363 | float | km/s | Amplitude-over-noise of emission line [OI] 6363 | |||
| V_NII_6547 | float | km/s | Velocity of emission line [NII] 6547 | |||
| V_NII_6547_Err | float | km/s | Error in velocity of emission line [NII] 6547 | |||
| Sigma_NII_6547 | float | km/s | Velocity dispersion of emission line [NII] 6547 | |||
| Sigma_NII_6547_Err | float | km/s | Error in velocity dispersion of emission line [NII] 6547 | |||
| Amplitude_NII_6547 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line [NII] 6547 | |||
| Amplitude_NII_6547_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line [NII] 6547 | |||
| Flux_NII_6547 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line [NII] 6547 | |||
| Flux_NII_6547_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line [NII] 6547 | |||
| EW_NII_6547 | float | Angstroms | Equivalent width of emission line [NII] 6547 | |||
| EW_NII_6547_Err | float | Angstroms | Error in equivalent width of emission line [NII] 6547 | |||
| Flux_Cont_NII_6547 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line [NII] 6547 | |||
| Flux_Cont_NII_6547_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line [NII] 6547 | |||
| Fit_Warning_NII_6547 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| V_Ha_6562 | float | km/s | Velocity of emission line Ha 6562 | |||
| V_Ha_6562_Err | float | km/s | Error in velocity of emission line Ha 6562 | |||
| Sigma_Ha_6562 | float | km/s | Velocity dispersion of emission line Ha 6562 | |||
| Sigma_Ha_6562_Err | float | km/s | Error in velocity dispersion of emission line Ha 6562 | |||
| Amplitude_Ha_6562 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line Ha 6562 | |||
| Amplitude_Ha_6562_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line Ha 6562 | |||
| Flux_Ha_6562 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line Ha 6562 | |||
| Flux_Ha_6562_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line Ha 6562 | |||
| EW_Ha_6562 | float | Angstroms | Equivalent width of emission line Ha 6562 | |||
| EW_Ha_6562_Err | float | Angstroms | Error in equivalent width of emission line Ha 6562 | |||
| Flux_Cont_Ha_6562 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line Ha 6562 | |||
| Flux_Cont_Ha_6562_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line Ha 6562 | |||
| Fit_Warning_Ha_6562 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| AoN_Ha_6562 | float | km/s | Amplitude-over-noise of emission line Ha 6562 | |||
| V_NII_6583 | float | km/s | Velocity of emission line [NII] 6583 | |||
| V_NII_6583_Err | float | km/s | Error in velocity of emission line [NII] 6583 | |||
| Sigma_NII_6583 | float | km/s | Velocity dispersion of emission line [NII] 6583 | |||
| Sigma_NII_6583_Err | float | km/s | Error in velocity dispersion of emission line [NII] 6583 | |||
| Amplitude_NII_6583 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line [NII] 6583 | |||
| Amplitude_NII_6583_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line [NII] 6583 | |||
| Flux_NII_6583 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line [NII] 6583 | |||
| Flux_NII_6583_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line [NII] 6583 | |||
| EW_NII_6583 | float | Angstroms | Equivalent width of emission line [NII] 6583 | |||
| EW_NII_6583_Err | float | Angstroms | Error in equivalent width of emission line [NII] 6583 | |||
| Flux_Cont_NII_6583 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line [NII] 6583 | |||
| Flux_Cont_NII_6583_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line [NII] 6583 | |||
| Fit_Warning_NII_6583 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| AoN_NII_6583 | float | km/s | Amplitude-over-noise of emission line [NII] 6583 | |||
| V_SII_6716 | float | km/s | Velocity of emission line [SII] 6716 | |||
| V_SII_6716_Err | float | km/s | Error in velocity of emission line [SII] 6716 | |||
| Sigma_SII_6716 | float | km/s | Velocity dispersion of emission line [SII] 6716 | |||
| Sigma_SII_6716_Err | float | km/s | Error in velocity dispersion of emission line [SII] 6716 | |||
| Amplitude_SII_6716 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line [SII] 6716 | |||
| Amplitude_SII_6716_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line [SII] 6716 | |||
| Flux_SII_6716 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line [SII] 6716 | |||
| Flux_SII_6716_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line [SII] 6716 | |||
| EW_SII_6716 | float | Angstroms | Equivalent width of emission line [SII] 6716 | |||
| EW_SII_6716_Err | float | Angstroms | Error in equivalent width of emission line [SII] 6716 | |||
| Flux_Cont_SII_6716 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line [SII] 6716 | |||
| Flux_Cont_SII_6716_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line [SII] 6716 | |||
| Fit_Warning_SII_6716 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| AoN_SII_6716 | float | km/s | Amplitude-over-noise of emission line [SII] 6716 | |||
| V_SII_6730 | float | km/s | Velocity of emission line [SII] 6730 | |||
| V_SII_6730_Err | float | km/s | Error in velocity of emission line [SII] 6730 | |||
| Sigma_SII_6730 | float | km/s | Velocity dispersion of emission line [SII] 6730 | |||
| Sigma_SII_6730_Err | float | km/s | Error in velocity dispersion of emission line [SII] 6730 | |||
| Amplitude_SII_6730 | float | 10^-17 ergs/cm^2/s/A | Amplitude of emission line [SII] 6730 | |||
| Amplitude_SII_6730_Err | float | 10^-17 ergs/cm^2/s/A | Error in amplitude of emission line [SII] 6730 | |||
| Flux_SII_6730 | float | 10^-17 ergs/cm^2/s/A | Flux of emission line [SII] 6730 | |||
| Flux_SII_6730_Err | float | 10^-17 ergs/cm^2/s/A | Error in flux of emission line [SII] 6730 | |||
| EW_SII_6730 | float | Angstroms | Equivalent width of emission line [SII] 6730 | |||
| EW_SII_6730_Err | float | Angstroms | Error in equivalent width of emission line [SII] 6730 | |||
| Flux_Cont_SII_6730 | float | 10^-17 ergs/cm^2/s/A | Continuum flux at wavelength of emission line [SII] 6730 | |||
| Flux_Cont_SII_6730_Err | float | 10^-17 ergs/cm^2/s/A | Error in continuum flux at wavelength of emission line [SII] 6730 | |||
| Fit_Warning_SII_6730 | int | Set to 1 if the emission line falls on a sky line (5577, 6300 or 6363), measurements set to zero in this case; otherwise, this flag is set to 0 | ||||
| AoN_SII_6730 | float | km/s | Amplitude-over-noise of emission line [SII] 6730 |
Estimated physical parameters for all galaxies in the MPA-JHU spectroscopic catalogue
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| specObjID | long | Unique ID | ||||
| bptclass | int | Emission line classification based on the BPT diagram using the methodology described in Brinchmann et al (2004). -1 means unclassifiable, 1 is star-forming, 2 means low S/N star-forming, 3 is composite, 4 AGN (excluding liners) and 5 is a low S/N LINER. | ||||
| oh_p2p5 | float | The 2.5 percentile of the Oxygen abundance derived using Charlot & Longhetti models. The values are reported as 12 + Log O/H. See Tremonti et al (2004) and Brinchmann et al (2004) for details. | ||||
| oh_p16 | float | The 16 percentile of the Oxygen abundance derived using Charlot & Longhetti models. The values are reported as 12 + Log O/H. See Tremonti et al (2004) and Brinchmann et al (2004) for details. | ||||
| oh_p50 | float | The median estimate of the Oxygen abundance derived using Charlot & Longhetti models. The values are reported as 12 + Log O/H. See Tremonti et al (2004) and Brinchmann et al (2004) for details. | ||||
| oh_p84 | float | The 84th percentile of the Oxygen abundance derived using Charlot & Longhetti models. The values are reported as 12 + Log O/H. See Tremonti et al (2004) and Brinchmann et al (2004) for details. | ||||
| oh_p97p5 | float | The 97.5 percentile of the Oxygen abundance derived using Charlot & Longhetti models. The values are reported as 12 + Log O/H. See Tremonti et al (2004) and Brinchmann et al (2004) for details. | ||||
| oh_entropy | float | The entropy (Sum p*lg(p)) of the PDF of 12 + Log O/H | ||||
| lgm_tot_p2p5 | float | Log solar masses | The 2.5 percentile of the Log total stellar mass PDF using model photometry. | |||
| lgm_tot_p16 | float | Log solar masses | The 16th percentile of the Log total stellar mass PDF using model photometry. | |||
| lgm_tot_p50 | float | Log solar masses | The median estimate of the Log total stellar mass PDF using model photometry. | |||
| lgm_tot_p84 | float | Log solar masses | The 84th percentile of the Log total stellar mass PDF using model photometry. | |||
| lgm_tot_p97p5 | float | Log solar masses | The 97.5 percentile of the Log total stellar mass PDF using model photometry. | |||
| lgm_fib_p2p5 | float | Log solar masses | The 2.5 percentile of the Log stellar mass within the fibre PDF using fibre photometry. | |||
| lgm_fib_p16 | float | Log solar masses | The 16th percentile of the Log stellar mass within the fibre PDF using fibre photometry. | |||
| lgm_fib_p50 | float | Log solar masses | The median estimate of the Log stellar mass within the fibre PDF using fibre photometry. | |||
| lgm_fib_p84 | float | Log solar masses | The 84th percentile of the Log stellar mass within the fibre PDF using fibre photometry. | |||
| lgm_fib_p97p5 | float | Log solar masses | The 97.5 percentile of the Log stellar mass within the fibre PDF using fibre photometry. | |||
| sfr_tot_p2p5 | float | Log Msun/yr | The 2.5 percentile of the Log total SFR PDF. This is derived by combining emission line measurements from within the fibre where possible and aperture corrections are done by fitting models ala Gallazzi et al (2005), Salim et al (2007) to the photometry outside the fibre. For those objects where the emission lines within the fibre do not provide an estimate of the SFR, model fits were made to the integrated photometry. | |||
| sfr_tot_p16 | float | Log Msun/yr | The 16th percentile of the Log total SFR PDF. This is derived by combining emission line measurements from within the fibre where possible and aperture corrections are done by fitting models ala Gallazzi et al (2005), Salim et al (2007) to the photometry outside the fibre. For those objects where the emission lines within the fibre do not provide an estimate of the SFR, model fits were made to the integrated photometry. | |||
| sfr_tot_p50 | float | Log Msun/yr | The median estimate of the Log total SFR PDF. This is derived by combining emission line measurements from within the fibre where possible and aperture corrections are done by fitting models ala Gallazzi et al (2005), Salim et al (2007) to the photometry outside the fibre. For those objects where the emission lines within the fibre do not provide an estimate of the SFR, model fits were made to the integrated photometry. | |||
| sfr_tot_p84 | float | Log Msun/yr | The 84th percentile of the Log total SFR PDF. This is derived by combining emission line measurements from within the fibre where possible and aperture corrections are done by fitting models ala Gallazzi et al (2005), Salim et al (2007) to the photometry outside the fibre. For those objects where the emission lines within the fibre do not provide an estimate of the SFR, model fits were made to the integrated photometry. | |||
| sfr_tot_p97p5 | float | Log Msun/yr | The 97.5 percentile of the Log total SFR PDF. This is derived by combining emission line measurements from within the fibre where possible and aperture corrections are done by fitting models ala Gallazzi et al (2005), Salim et al (2007) to the photometry outside the fibre. For those objects where the emission lines within the fibre do not provide an estimate of the SFR, model fits were made to the integrated photometry. | |||
| sfr_tot_entropy | float | The entropy (Sum p*lg(p)) of the PDF of the total SFR | ||||
| sfr_fib_p2p5 | float | Log Msun/yr | The 2.5 percentile of the Log SFR within the fiber PDF. For galaxies of the star-forming class, emission lines were used (c.f. Brinchmann et al 2004) while for others models were fit to the fibre photometry.. | |||
| sfr_fib_p16 | float | Log Msun/yr | The 16th percentile of the Log SFR within the fiber PDF. For galaxies of the star-forming class, emission lines were used (c.f. Brinchmann et al 2004) while for others models were fit to the fibre photometry.. | |||
| sfr_fib_p50 | float | Log Msun/yr | The median estimate of the Log SFR within the fiber PDF. For galaxies of the star-forming class, emission lines were used (c.f. Brinchmann et al 2004) while for others models were fit to the fibre photometry.. | |||
| sfr_fib_p84 | float | Log Msun/yr | The 84th percentile of the Log SFR within the fiber PDF. For galaxies of the star-forming class, emission lines were used (c.f. Brinchmann et al 2004) while for others models were fit to the fibre photometry.. | |||
| sfr_fib_p97p5 | float | Log Msun/yr | The 97.5 percentile of the Log SFR within the fiber PDF. For galaxies of the star-forming class, emission lines were used (c.f. Brinchmann et al 2004) while for others models were fit to the fibre photometry.. | |||
| sfr_fib_entropy | float | The entropy (Sum p*lg(p)) of the PDF of the fiber SFR | ||||
| specsfr_tot_p2p5 | float | Log Msun/yr | The 2.5 percentile of the Log total SPECSFR PDF. This is derived by combining emission line measurements from within the fibre where possible and aperture corrections are done by fitting models ala Gallazzi et al (2005), Salim et al (2007) to the photometry outside the fibre. For those objects where the emission lines within the fibre do not provide an estimate of the SFR, model fits were made to the integrated photometry. | |||
| specsfr_tot_p16 | float | Log Msun/yr | The 16th percentile of the Log total SPECSFR PDF. This is derived by combining emission line measurements from within the fibre where possible and aperture corrections are done by fitting models ala Gallazzi et al (2005), Salim et al (2007) to the photometry outside the fibre. For those objects where the emission lines within the fibre do not provide an estimate of the SFR, model fits were made to the integrated photometry. | |||
| specsfr_tot_p50 | float | Log Msun/yr | The median estimate of the Log total SPECSFR PDF. This is derived by combining emission line measurements from within the fibre where possible and aperture corrections are done by fitting models ala Gallazzi et al (2005), Salim et al (2007) to the photometry outside the fibre. For those objects where the emission lines within the fibre do not provide an estimate of the SFR, model fits were made to the integrated photometry. | |||
| specsfr_tot_p84 | float | Log Msun/yr | The 84th percentile of the Log total SPECSFR PDF. This is derived by combining emission line measurements from within the fibre where possible and aperture corrections are done by fitting models ala Gallazzi et al (2005), Salim et al (2007) to the photometry outside the fibre. For those objects where the emission lines within the fibre do not provide an estimate of the SFR, model fits were made to the integrated photometry. | |||
| specsfr_tot_p97p5 | float | Log Msun/yr | The 97.5 percentile of the Log total SPECSFR PDF. This is derived by combining emission line measurements from within the fibre where possible and aperture corrections are done by fitting models ala Gallazzi et al (2005), Salim et al (2007) to the photometry outside the fibre. For those objects where the emission lines within the fibre do not provide an estimate of the SFR, model fits were made to the integrated photometry. | |||
| specsfr_tot_entropy | float | The entropy (Sum p*lg(p)) of the PDF of the total SPECSFR | ||||
| specsfr_fib_p2p5 | float | Log Msun/yr | The 2.5 percentile of the Log SPECSFR within the fiber PDF. For galaxies of the star-forming class, emission lines were used (c.f. Brinchmann et al 2004) while for others models were fit to the fibre photometry.. | |||
| specsfr_fib_p16 | float | Log Msun/yr | The 16th percentile of the Log SPECSFR within the fiber PDF. For galaxies of the star-forming class, emission lines were used (c.f. Brinchmann et al 2004) while for others models were fit to the fibre photometry.. | |||
| specsfr_fib_p50 | float | Log Msun/yr | The median estimate of the Log SPECSFR within the fiber PDF. For galaxies of the star-forming class, emission lines were used (c.f. Brinchmann et al 2004) while for others models were fit to the fibre photometry.. | |||
| specsfr_fib_p84 | float | Log Msun/yr | The 84th percentile of the Log SPECSFR within the fiber PDF. For galaxies of the star-forming class, emission lines were used (c.f. Brinchmann et al 2004) while for others models were fit to the fibre photometry.. | |||
| specsfr_fib_p97p5 | float | Log Msun/yr | The 97.5 percentile of the Log SPECSFR within the fiber PDF. For galaxies of the star-forming class, emission lines were used (c.f. Brinchmann et al 2004) while for others models were fit to the fibre photometry.. | |||
| specsfr_fib_entropy | float | The entropy (Sum p*lg(p)) of the PDF of the fiber SPECSFR |
Index measurements of spectra from the MPA-JHU spectroscopic catalogue
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| specObjID | long | Unique ID | ||||
| lick_cn1 | float | mag | Restframe index measurement | |||
| lick_cn1_err | float | mag | Error on index measurement | |||
| lick_cn1_model | float | mag | Index of best fit model spectrum | |||
| lick_cn1_sub | float | mag | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| lick_cn1_sub_err | float | mag | Error in the above index measurement | |||
| lick_cn2 | float | mag | Restframe index measurement | |||
| lick_cn2_err | float | mag | Error on index measurement | |||
| lick_cn2_model | float | mag | Index of best fit model spectrum | |||
| lick_cn2_sub | float | mag | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| lick_cn2_sub_err | float | mag | Error in the above index measurement | |||
| lick_ca4227 | float | A | Restframe index measurement | |||
| lick_ca4227_err | float | A | Error on index measurement | |||
| lick_ca4227_model | float | A | Index of best fit model spectrum | |||
| lick_ca4227_sub | float | A | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| lick_ca4227_sub_err | float | A | Error in the above index measurement | |||
| lick_g4300 | float | A | Restframe index measurement | |||
| lick_g4300_err | float | A | Error on index measurement | |||
| lick_g4300_model | float | A | Index of best fit model spectrum | |||
| lick_g4300_sub | float | A | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| lick_g4300_sub_err | float | A | Error in the above index measurement | |||
| lick_fe4383 | float | A | Restframe index measurement | |||
| lick_fe4383_err | float | A | Error on index measurement | |||
| lick_fe4383_model | float | A | Index of best fit model spectrum | |||
| lick_fe4383_sub | float | A | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| lick_fe4383_sub_err | float | A | Error in the above index measurement | |||
| lick_ca4455 | float | A | Restframe index measurement | |||
| lick_ca4455_err | float | A | Error on index measurement | |||
| lick_ca4455_model | float | A | Index of best fit model spectrum | |||
| lick_ca4455_sub | float | A | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| lick_ca4455_sub_err | float | A | Error in the above index measurement | |||
| lick_fe4531 | float | A | Restframe index measurement | |||
| lick_fe4531_err | float | A | Error on index measurement | |||
| lick_fe4531_model | float | A | Index of best fit model spectrum | |||
| lick_fe4531_sub | float | A | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| lick_fe4531_sub_err | float | A | Error in the above index measurement | |||
| lick_c4668 | float | A | Restframe index measurement | |||
| lick_c4668_err | float | A | Error on index measurement | |||
| lick_c4668_model | float | A | Index of best fit model spectrum | |||
| lick_c4668_sub | float | A | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| lick_c4668_sub_err | float | A | Error in the above index measurement | |||
| lick_hb | float | A | Restframe index measurement | |||
| lick_hb_err | float | A | Error on index measurement | |||
| lick_hb_model | float | A | Index of best fit model spectrum | |||
| lick_hb_sub | float | A | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| lick_hb_sub_err | float | A | Error in the above index measurement | |||
| lick_fe5015 | float | A | Restframe index measurement | |||
| lick_fe5015_err | float | A | Error on index measurement | |||
| lick_fe5015_model | float | A | Index of best fit model spectrum | |||
| lick_fe5015_sub | float | A | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| lick_fe5015_sub_err | float | A | Error in the above index measurement | |||
| lick_mg1 | float | mag | Restframe index measurement | |||
| lick_mg1_err | float | mag | Error on index measurement | |||
| lick_mg1_model | float | mag | Index of best fit model spectrum | |||
| lick_mg1_sub | float | mag | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| lick_mg1_sub_err | float | mag | Error in the above index measurement | |||
| lick_mg2 | float | mag | Restframe index measurement | |||
| lick_mg2_err | float | mag | Error on index measurement | |||
| lick_mg2_model | float | mag | Index of best fit model spectrum | |||
| lick_mg2_sub | float | mag | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| lick_mg2_sub_err | float | mag | Error in the above index measurement | |||
| lick_mgb | float | A | Restframe index measurement | |||
| lick_mgb_err | float | A | Error on index measurement | |||
| lick_mgb_model | float | A | Index of best fit model spectrum | |||
| lick_mgb_sub | float | A | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| lick_mgb_sub_err | float | A | Error in the above index measurement | |||
| lick_fe5270 | float | A | Restframe index measurement | |||
| lick_fe5270_err | float | A | Error on index measurement | |||
| lick_fe5270_model | float | A | Index of best fit model spectrum | |||
| lick_fe5270_sub | float | A | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| lick_fe5270_sub_err | float | A | Error in the above index measurement | |||
| lick_fe5335 | float | A | Restframe index measurement | |||
| lick_fe5335_err | float | A | Error on index measurement | |||
| lick_fe5335_model | float | A | Index of best fit model spectrum | |||
| lick_fe5335_sub | float | A | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| lick_fe5335_sub_err | float | A | Error in the above index measurement | |||
| lick_fe5406 | float | A | Restframe index measurement | |||
| lick_fe5406_err | float | A | Error on index measurement | |||
| lick_fe5406_model | float | A | Index of best fit model spectrum | |||
| lick_fe5406_sub | float | A | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| lick_fe5406_sub_err | float | A | Error in the above index measurement | |||
| lick_fe5709 | float | A | Restframe index measurement | |||
| lick_fe5709_err | float | A | Error on index measurement | |||
| lick_fe5709_model | float | A | Index of best fit model spectrum | |||
| lick_fe5709_sub | float | A | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| lick_fe5709_sub_err | float | A | Error in the above index measurement | |||
| lick_fe5782 | float | A | Restframe index measurement | |||
| lick_fe5782_err | float | A | Error on index measurement | |||
| lick_fe5782_model | float | A | Index of best fit model spectrum | |||
| lick_fe5782_sub | float | A | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| lick_fe5782_sub_err | float | A | Error in the above index measurement | |||
| lick_nad | float | A | Restframe index measurement | |||
| lick_nad_err | float | A | Error on index measurement | |||
| lick_nad_model | float | A | Index of best fit model spectrum | |||
| lick_nad_sub | float | A | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| lick_nad_sub_err | float | A | Error in the above index measurement | |||
| lick_tio1 | float | mag | Restframe index measurement | |||
| lick_tio1_err | float | mag | Error on index measurement | |||
| lick_tio1_model | float | mag | Index of best fit model spectrum | |||
| lick_tio1_sub | float | mag | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| lick_tio1_sub_err | float | mag | Error in the above index measurement | |||
| lick_tio2 | float | mag | Restframe index measurement | |||
| lick_tio2_err | float | mag | Error on index measurement | |||
| lick_tio2_model | float | mag | Index of best fit model spectrum | |||
| lick_tio2_sub | float | mag | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| lick_tio2_sub_err | float | mag | Error in the above index measurement | |||
| lick_hd_a | float | A | Restframe index measurement | |||
| lick_hd_a_err | float | A | Error on index measurement | |||
| lick_hd_a_model | float | A | Index of best fit model spectrum | |||
| lick_hd_a_sub | float | A | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| lick_hd_a_sub_err | float | A | Error in the above index measurement | |||
| lick_hg_a | float | A | Restframe index measurement | |||
| lick_hg_a_err | float | A | Error on index measurement | |||
| lick_hg_a_model | float | A | Index of best fit model spectrum | |||
| lick_hg_a_sub | float | A | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| lick_hg_a_sub_err | float | A | Error in the above index measurement | |||
| lick_hd_f | float | A | Restframe index measurement | |||
| lick_hd_f_err | float | A | Error on index measurement | |||
| lick_hd_f_model | float | A | Index of best fit model spectrum | |||
| lick_hd_f_sub | float | A | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| lick_hd_f_sub_err | float | A | Error in the above index measurement | |||
| lick_hg_f | float | A | Restframe index measurement | |||
| lick_hg_f_err | float | A | Error on index measurement | |||
| lick_hg_f_model | float | A | Index of best fit model spectrum | |||
| lick_hg_f_sub | float | A | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| lick_hg_f_sub_err | float | A | Error in the above index measurement | |||
| dtt_caii8498 | float | A | Restframe index measurement | |||
| dtt_caii8498_err | float | A | Error on index measurement | |||
| dtt_caii8498_model | float | A | Index of best fit model spectrum | |||
| dtt_caii8498_sub | float | A | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| dtt_caii8498_sub_err | float | A | Error in the above index measurement | |||
| dtt_caii8542 | float | A | Restframe index measurement | |||
| dtt_caii8542_err | float | A | Error on index measurement | |||
| dtt_caii8542_model | float | A | Index of best fit model spectrum | |||
| dtt_caii8542_sub | float | A | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| dtt_caii8542_sub_err | float | A | Error in the above index measurement | |||
| dtt_caii8662 | float | A | Restframe index measurement | |||
| dtt_caii8662_err | float | A | Error on index measurement | |||
| dtt_caii8662_model | float | A | Index of best fit model spectrum | |||
| dtt_caii8662_sub | float | A | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| dtt_caii8662_sub_err | float | A | Error in the above index measurement | |||
| dtt_mgi8807 | float | A | Restframe index measurement | |||
| dtt_mgi8807_err | float | A | Error on index measurement | |||
| dtt_mgi8807_model | float | A | Index of best fit model spectrum | |||
| dtt_mgi8807_sub | float | A | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| dtt_mgi8807_sub_err | float | A | Error in the above index measurement | |||
| bh_cnb | float | mag | Restframe index measurement | |||
| bh_cnb_err | float | mag | Error on index measurement | |||
| bh_cnb_model | float | mag | Index of best fit model spectrum | |||
| bh_cnb_sub | float | mag | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| bh_cnb_sub_err | float | mag | Error in the above index measurement | |||
| bh_hk | float | mag | Restframe index measurement | |||
| bh_hk_err | float | mag | Error on index measurement | |||
| bh_hk_model | float | mag | Index of best fit model spectrum | |||
| bh_hk_sub | float | mag | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| bh_hk_sub_err | float | mag | Error in the above index measurement | |||
| bh_cai | float | mag | Restframe index measurement | |||
| bh_cai_err | float | mag | Error on index measurement | |||
| bh_cai_model | float | mag | Index of best fit model spectrum | |||
| bh_cai_sub | float | mag | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| bh_cai_sub_err | float | mag | Error in the above index measurement | |||
| bh_g | float | mag | Restframe index measurement | |||
| bh_g_err | float | mag | Error on index measurement | |||
| bh_g_model | float | mag | Index of best fit model spectrum | |||
| bh_g_sub | float | mag | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| bh_g_sub_err | float | mag | Error in the above index measurement | |||
| bh_hb | float | mag | Restframe index measurement | |||
| bh_hb_err | float | mag | Error on index measurement | |||
| bh_hb_model | float | mag | Index of best fit model spectrum | |||
| bh_hb_sub | float | mag | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| bh_hb_sub_err | float | mag | Error in the above index measurement | |||
| bh_mgg | float | mag | Restframe index measurement | |||
| bh_mgg_err | float | mag | Error on index measurement | |||
| bh_mgg_model | float | mag | Index of best fit model spectrum | |||
| bh_mgg_sub | float | mag | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| bh_mgg_sub_err | float | mag | Error in the above index measurement | |||
| bh_mh | float | mag | Restframe index measurement | |||
| bh_mh_err | float | mag | Error on index measurement | |||
| bh_mh_model | float | mag | Index of best fit model spectrum | |||
| bh_mh_sub | float | mag | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| bh_mh_sub_err | float | mag | Error in the above index measurement | |||
| bh_fc | float | mag | Restframe index measurement | |||
| bh_fc_err | float | mag | Error on index measurement | |||
| bh_fc_model | float | mag | Index of best fit model spectrum | |||
| bh_fc_sub | float | mag | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| bh_fc_sub_err | float | mag | Error in the above index measurement | |||
| bh_nad | float | mag | Restframe index measurement | |||
| bh_nad_err | float | mag | Error on index measurement | |||
| bh_nad_model | float | mag | Index of best fit model spectrum | |||
| bh_nad_sub | float | mag | Restframe index measurement on the data after subtracting all 3-sigma emission lines | |||
| bh_nad_sub_err | float | mag | Error in the above index measurement | |||
| d4000 | float | 4000AA break, Bruzual (1983) definition | ||||
| d4000_err | float | Uncertainty estimate for 4000AA break, Bruzual (1983) definition | ||||
| d4000_model | float | 4000AA break, Bruzual (1983) definition measured off best-fit CB08 model | ||||
| d4000_sub | float | 4000AA break, Bruzual (1983) definition after correction for emission lines | ||||
| d4000_sub_err | float | Uncertainty estimate for 4000AA break, Bruzual (1983) definition after correction for emission lines | ||||
| d4000_n | float | 4000AA break, Balogh et al (1999) definition | ||||
| d4000_n_err | float | Uncertainty estimate for 4000AA break, Balogh et al (1999) definition | ||||
| d4000_n_model | float | 4000AA break, Balogh et al (1999) definition measured off best-fit CB08 model | ||||
| d4000_n_sub | float | 4000AA break, Balogh et al (1999) definition after correction for emission lines | ||||
| d4000_n_sub_err | float | Uncertainty estimate for 4000AA break, Balogh et al (1999) definition after correction for emission lines | ||||
| d4000_red | float | The flux in the red window of the Bruzual (1983) definition of D4000 | ||||
| d4000_blue | float | The flux in the blue window of the Bruzual (1983) definition of D4000 | ||||
| d4000_n_red | float | The flux in the red window of the Balogh et al (1999) definition of D4000 | ||||
| d4000_n_blue | float | The flux in the blue window of the Balogh et al (1999) definition of D4000 | ||||
| d4000_sub_red | float | The flux in the red window of the Bruzual (1983) definition of D4000 after subtraction of emission lines | ||||
| d4000_sub_blue | float | The flux in the blue window of the Bruzual (1983) definition of D4000 after subtraction of emission lines | ||||
| d4000_n_sub_red | float | The flux in the red window of the Balogh et al (1999) definition of D4000 after subtraction of emission lines | ||||
| d4000_n_sub_blue | float | The flux in the blue window of the Balogh et al (1999)q definition of D4000 after subtraction of emission lines | ||||
| tauv_model_040 | float | Dust attenuation of the best fit Z=0.004 CB08 model | ||||
| model_coef_040 | float | The scaling coefficients of the best fit Z=0.004 CB08 model | ||||
| model_chisq_040 | float | The chi^2 of the best fit Z=0.004 CB08 model | ||||
| tauv_model_080 | float | Dust attenuation of the best fit Z=0.008 CB08 model | ||||
| model_coef_080 | float | The scaling coefficients of the best fit Z=0.008 CB08 model | ||||
| model_chisq_080 | float | The chi^2 of the best fit Z=0.008 CB08 model | ||||
| tauv_model_170 | float | Dust attenuation of the best fit Z=0.017 CB08 model | ||||
| model_coef_170 | float | The scaling coefficients of the best fit Z=0.017 CB08 model | ||||
| model_chisq_170 | float | The chi^2 of the best fit Z=0.017 CB08 model | ||||
| tauv_model_400 | float | Dust attenuation of the best fit Z=0.04 CB08 model | ||||
| model_coef_400 | float | The scaling coefficients of the best fit Z=0.04 CB08 model | ||||
| model_chisq_400 | float | The chi^2 of the best fit Z=0.04 CB08 model | ||||
| best_model_z | float | Metallicity of best fitting (min chisq) model Z = 0.004 / 0.017 / 0.050 (0.2 1.0, 2.5 x solar) | ||||
| tauv_cont | float | V-band optical depth (TauV = A_V / 1.086) affecting the stars from best fit model (best of 4 Z's) | ||||
| model_coef | float | Coeficients of best fit model (best of 4 Z's) | ||||
| model_chisq | float | Reduced chi-squared of best fit model (best of 4 Z's) |
General information for the MPA-JHU spectroscopic re-analysi
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| specObjID | long | Unique ID | ||||
| plateid | int | Plate number | ||||
| mjd | int | Modified Julian Date of plate observation | ||||
| fiberid | int | Fiber number (1 - 640) | ||||
| ra | float | deg | Right Ascention of drilled fiber position | |||
| dec | float | deg | Declination of drilled fiber position | |||
| primtarget | int | Primary Target Flag (MAIN galaxy = 64) | ||||
| sectarget | int | Secondary Target Flag (QA = 8) | ||||
| targettype | string | Text version of primary target (GALAXY/QA/QSO/ROSAT_D) | ||||
| spectrotype | string | Schlegel classification of spectrum ... code is only run where this is set to "GALAXY" | ||||
| subclass | string | Schlegel subclass from PCA analysis -- not alwasy correct!! AGN/BROADLINE/STARBURST/STARFORMING | ||||
| z | float | Redshift from Schlegel | ||||
| z_err | float | Redshift error | ||||
| z_warning | int | Bad redshift if this is non-zero -- see Schlegel data model | ||||
| v_disp | float | km/s | Velocity dispersion from Schlegel | |||
| v_disp_err | float | km/s | Velocity dispersion error (negative for invalid fit) | |||
| sn_median | float | Median S/N per pixel of the whole spectrum | ||||
| e_bv_sfd | float | E(B-V) of foreground reddening from SFD maps | ||||
| release | string | Data Release (dr1/dr2/dr3/dr4) | ||||
| reliable | int | has "reliable" line measurements and physical parameters |
Emission line measurements from MPA-JHU spectroscopic reanalysi
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| specObjID | long | Unique ID | ||||
| sigma_balmer | float | km/s | Velocity dispersion (sigma not FWHM) measured simultaneously in all of the Balmer lines | |||
| sigma_balmer_err | float | km/s | Error in the above | |||
| sigma_forbidden | float | km/s | Velocity dispersion (sigma not FWHM) measured simultaneously in all the forbidden lines | |||
| sigma_forbidden_err | float | km/s | Error in the above | |||
| v_off_balmer | float | km/s | Velocity offset of the Balmer lines from the measured redshift | |||
| v_off_balmer_err | float | km/s | Error in the above | |||
| v_off_forbidden | float | km/s | Velocity offset of the forbidden lines from the measured redshift | |||
| v_off_forbidden_err | float | km/s | Error in the above | |||
| oii_3726_cont | float | 1e-17 erg/s/cm^2/AA | Continuum at line center from 200 pixel median smoothing of the emission-line subtracted continuum | |||
| oii_3726_cont_err | float | 1e-17 erg/s/cm^2/AA | Error in the continuum computed from the variance in the band pass | |||
| oii_3726_reqw | float | Ang | The equivalent width of the continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative). In this case the continuum comes from a running 200 pixel median and does not properly account for stellar absorption. In general the EQW measurements provide a better measure of the true equivalent width. The purpose of this measurement is to help characterize the stellar absorption effecting the line. (EW_stellar = REQW - EQW) | |||
| oii_3726_reqw_err | float | Ang | Error in the equivalent width described above | |||
| oii_3726_eqw | float | Ang | The equivalent width of the CB08 continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative) . This properly takes into account stellar absorption. Note that it will not be correct in the case of blended lines (ie NII & H-alpha) -- instead use FLUX/CONT. | |||
| oii_3726_eqw_err | float | Ang | Error in the equivalent width described above | |||
| oii_3726_flux | float | 1e-17 erg/s/cm^2 | Flux from Gaussian fit to continuum subtracted data. (Note that the fit is done simultaneously to all the lines so de-blending happens automatically) | |||
| oii_3726_flux_err | float | 1e-17 erg/s/cm^2 | Error in the flux | |||
| oii_3726_inst_res | float | km/s | Instrumental resolution at the line center (measured for each spectrum from the ARC lamps) | |||
| oii_3726_chisq | float | Reduced chi-squared of the line fit over the bandpass used for the EW measurement | ||||
| oii_3729_cont | float | 1e-17 erg/s/cm^2/AA | Continuum at line center from 200 pixel median smoothing of the emission-line subtracted continuum | |||
| oii_3729_cont_err | float | 1e-17 erg/s/cm^2/AA | Error in the continuum computed from the variance in the band pass | |||
| oii_3729_reqw | float | Ang | The equivalent width of the continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative). In this case the continuum comes from a running 200 pixel median and does not properly account for stellar absorption. In general the EQW measurements provide a better measure of the true equivalent width. The purpose of this measurement is to help characterize the stellar absorption effecting the line. (EW_stellar = REQW - EQW) | |||
| oii_3729_reqw_err | float | Ang | Error in the equivalent width described above | |||
| oii_3729_eqw | float | Ang | The equivalent width of the CB08 continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative) . This properly takes into account stellar absorption. Note that it will not be correct in the case of blended lines (ie NII & H-alpha) -- instead use FLUX/CONT. | |||
| oii_3729_eqw_err | float | Ang | Error in the equivalent width described above | |||
| oii_3729_flux | float | 1e-17 erg/s/cm^2 | Flux from Gaussian fit to continuum subtracted data. (Note that the fit is done simultaneously to all the lines so de-blending happens automatically) | |||
| oii_3729_flux_err | float | 1e-17 erg/s/cm^2 | Error in the flux | |||
| oii_3729_inst_res | float | km/s | Instrumental resolution at the line center (measured for each spectrum from the ARC lamps) | |||
| oii_3729_chisq | float | Reduced chi-squared of the line fit over the bandpass used for the EW measurement | ||||
| neiii_3869_cont | float | 1e-17 erg/s/cm^2/AA | Continuum at line center from 200 pixel median smoothing of the emission-line subtracted continuum | |||
| neiii_3869_cont_err | float | 1e-17 erg/s/cm^2/AA | Error in the continuum computed from the variance in the band pass | |||
| neiii_3869_reqw | float | Ang | The equivalent width of the continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative). In this case the continuum comes from a running 200 pixel median and does not properly account for stellar absorption. In general the EQW measurements provide a better measure of the true equivalent width. The purpose of this measurement is to help characterize the stellar absorption effecting the line. (EW_stellar = REQW - EQW) | |||
| neiii_3869_reqw_err | float | Ang | Error in the equivalent width described above | |||
| neiii_3869_eqw | float | Ang | The equivalent width of the CB08 continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative) . This properly takes into account stellar absorption. Note that it will not be correct in the case of blended lines (ie NII & H-alpha) -- instead use FLUX/CONT. | |||
| neiii_3869_eqw_err | float | Ang | Error in the equivalent width described above | |||
| neiii_3869_flux | float | 1e-17 erg/s/cm^2 | Flux from Gaussian fit to continuum subtracted data. (Note that the fit is done simultaneously to all the lines so de-blending happens automatically) | |||
| neiii_3869_flux_err | float | 1e-17 erg/s/cm^2 | Error in the flux | |||
| neiii_3869_inst_res | float | km/s | Instrumental resolution at the line center (measured for each spectrum from the ARC lamps) | |||
| neiii_3869_chisq | float | Reduced chi-squared of the line fit over the bandpass used for the EW measurement | ||||
| h_delta_cont | float | 1e-17 erg/s/cm^2/AA | Continuum at line center from 200 pixel median smoothing of the emission-line subtracted continuum | |||
| h_delta_cont_err | float | 1e-17 erg/s/cm^2/AA | Error in the continuum computed from the variance in the band pass | |||
| h_delta_reqw | float | Ang | The equivalent width of the continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative). In this case the continuum comes from a running 200 pixel median and does not properly account for stellar absorption. In general the EQW measurements provide a better measure of the true equivalent width. The purpose of this measurement is to help characterize the stellar absorption effecting the line. (EW_stellar = REQW - EQW) | |||
| h_delta_reqw_err | float | Ang | Error in the equivalent width described above | |||
| h_delta_eqw | float | Ang | The equivalent width of the CB08 continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative) . This properly takes into account stellar absorption. Note that it will not be correct in the case of blended lines (ie NII & H-alpha) -- instead use FLUX/CONT. | |||
| h_delta_eqw_err | float | Ang | Error in the equivalent width described above | |||
| h_delta_flux | float | 1e-17 erg/s/cm^2 | Flux from Gaussian fit to continuum subtracted data. (Note that the fit is done simultaneously to all the lines so de-blending happens automatically) | |||
| h_delta_flux_err | float | 1e-17 erg/s/cm^2 | Error in the flux | |||
| h_delta_inst_res | float | km/s | Instrumental resolution at the line center (measured for each spectrum from the ARC lamps) | |||
| h_delta_chisq | float | Reduced chi-squared of the line fit over the bandpass used for the EW measurement | ||||
| h_gamma_cont | float | 1e-17 erg/s/cm^2/AA | Continuum at line center from 200 pixel median smoothing of the emission-line subtracted continuum | |||
| h_gamma_cont_err | float | 1e-17 erg/s/cm^2/AA | Error in the continuum computed from the variance in the band pass | |||
| h_gamma_reqw | float | Ang | The equivalent width of the continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative). In this case the continuum comes from a running 200 pixel median and does not properly account for stellar absorption. In general the EQW measurements provide a better measure of the true equivalent width. The purpose of this measurement is to help characterize the stellar absorption effecting the line. (EW_stellar = REQW - EQW) | |||
| h_gamma_reqw_err | float | Ang | Error in the equivalent width described above | |||
| h_gamma_eqw | float | Ang | The equivalent width of the CB08 continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative) . This properly takes into account stellar absorption. Note that it will not be correct in the case of blended lines (ie NII & H-alpha) -- instead use FLUX/CONT. | |||
| h_gamma_eqw_err | float | Ang | Error in the equivalent width described above | |||
| h_gamma_flux | float | 1e-17 erg/s/cm^2 | Flux from Gaussian fit to continuum subtracted data. (Note that the fit is done simultaneously to all the lines so de-blending happens automatically) | |||
| h_gamma_flux_err | float | 1e-17 erg/s/cm^2 | Error in the flux | |||
| h_gamma_inst_res | float | km/s | Instrumental resolution at the line center (measured for each spectrum from the ARC lamps) | |||
| h_gamma_chisq | float | Reduced chi-squared of the line fit over the bandpass used for the EW measurement | ||||
| oiii_4363_cont | float | 1e-17 erg/s/cm^2/AA | Continuum at line center from 200 pixel median smoothing of the emission-line subtracted continuum | |||
| oiii_4363_cont_err | float | 1e-17 erg/s/cm^2/AA | Error in the continuum computed from the variance in the band pass | |||
| oiii_4363_reqw | float | Ang | The equivalent width of the continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative). In this case the continuum comes from a running 200 pixel median and does not properly account for stellar absorption. In general the EQW measurements provide a better measure of the true equivalent width. The purpose of this measurement is to help characterize the stellar absorption effecting the line. (EW_stellar = REQW - EQW) | |||
| oiii_4363_reqw_err | float | Ang | Error in the equivalent width described above | |||
| oiii_4363_eqw | float | Ang | The equivalent width of the CB08 continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative) . This properly takes into account stellar absorption. Note that it will not be correct in the case of blended lines (ie NII & H-alpha) -- instead use FLUX/CONT. | |||
| oiii_4363_eqw_err | float | Ang | Error in the equivalent width described above | |||
| oiii_4363_flux | float | 1e-17 erg/s/cm^2 | Flux from Gaussian fit to continuum subtracted data. (Note that the fit is done simultaneously to all the lines so de-blending happens automatically) | |||
| oiii_4363_flux_err | float | 1e-17 erg/s/cm^2 | Error in the flux | |||
| oiii_4363_inst_res | float | km/s | Instrumental resolution at the line center (measured for each spectrum from the ARC lamps) | |||
| oiii_4363_chisq | float | Reduced chi-squared of the line fit over the bandpass used for the EW measurement | ||||
| h_beta_cont | float | 1e-17 erg/s/cm^2/AA | Continuum at line center from 200 pixel median smoothing of the emission-line subtracted continuum | |||
| h_beta_cont_err | float | 1e-17 erg/s/cm^2/AA | Error in the continuum computed from the variance in the band pass | |||
| h_beta_reqw | float | Ang | The equivalent width of the continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative). In this case the continuum comes from a running 200 pixel median and does not properly account for stellar absorption. In general the EQW measurements provide a better measure of the true equivalent width. The purpose of this measurement is to help characterize the stellar absorption effecting the line. (EW_stellar = REQW - EQW) | |||
| h_beta_reqw_err | float | Ang | Error in the equivalent width described above | |||
| h_beta_eqw | float | Ang | The equivalent width of the CB08 continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative) . This properly takes into account stellar absorption. Note that it will not be correct in the case of blended lines (ie NII & H-alpha) -- instead use FLUX/CONT. | |||
| h_beta_eqw_err | float | Ang | Error in the equivalent width described above | |||
| h_beta_flux | float | 1e-17 erg/s/cm^2 | Flux from Gaussian fit to continuum subtracted data. (Note that the fit is done simultaneously to all the lines so de-blending happens automatically) | |||
| h_beta_flux_err | float | 1e-17 erg/s/cm^2 | Error in the flux | |||
| h_beta_inst_res | float | km/s | Instrumental resolution at the line center (measured for each spectrum from the ARC lamps) | |||
| h_beta_chisq | float | Reduced chi-squared of the line fit over the bandpass used for the EW measurement | ||||
| oiii_4959_cont | float | 1e-17 erg/s/cm^2/AA | Continuum at line center from 200 pixel median smoothing of the emission-line subtracted continuum | |||
| oiii_4959_cont_err | float | 1e-17 erg/s/cm^2/AA | Error in the continuum computed from the variance in the band pass | |||
| oiii_4959_reqw | float | Ang | The equivalent width of the continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative). In this case the continuum comes from a running 200 pixel median and does not properly account for stellar absorption. In general the EQW measurements provide a better measure of the true equivalent width. The purpose of this measurement is to help characterize the stellar absorption effecting the line. (EW_stellar = REQW - EQW) | |||
| oiii_4959_reqw_err | float | Ang | Error in the equivalent width described above | |||
| oiii_4959_eqw | float | Ang | The equivalent width of the CB08 continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative) . This properly takes into account stellar absorption. Note that it will not be correct in the case of blended lines (ie NII & H-alpha) -- instead use FLUX/CONT. | |||
| oiii_4959_eqw_err | float | Ang | Error in the equivalent width described above | |||
| oiii_4959_flux | float | 1e-17 erg/s/cm^2 | Flux from Gaussian fit to continuum subtracted data. (Note that the fit is done simultaneously to all the lines so de-blending happens automatically) | |||
| oiii_4959_flux_err | float | 1e-17 erg/s/cm^2 | Error in the flux | |||
| oiii_4959_inst_res | float | km/s | Instrumental resolution at the line center (measured for each spectrum from the ARC lamps) | |||
| oiii_4959_chisq | float | Reduced chi-squared of the line fit over the bandpass used for the EW measurement | ||||
| oiii_5007_cont | float | 1e-17 erg/s/cm^2/AA | Continuum at line center from 200 pixel median smoothing of the emission-line subtracted continuum | |||
| oiii_5007_cont_err | float | 1e-17 erg/s/cm^2/AA | Error in the continuum computed from the variance in the band pass | |||
| oiii_5007_reqw | float | Ang | The equivalent width of the continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative). In this case the continuum comes from a running 200 pixel median and does not properly account for stellar absorption. In general the EQW measurements provide a better measure of the true equivalent width. The purpose of this measurement is to help characterize the stellar absorption effecting the line. (EW_stellar = REQW - EQW) | |||
| oiii_5007_reqw_err | float | Ang | Error in the equivalent width described above | |||
| oiii_5007_eqw | float | Ang | The equivalent width of the CB08 continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative) . This properly takes into account stellar absorption. Note that it will not be correct in the case of blended lines (ie NII & H-alpha) -- instead use FLUX/CONT. | |||
| oiii_5007_eqw_err | float | Ang | Error in the equivalent width described above | |||
| oiii_5007_flux | float | 1e-17 erg/s/cm^2 | Flux from Gaussian fit to continuum subtracted data. (Note that the fit is done simultaneously to all the lines so de-blending happens automatically) | |||
| oiii_5007_flux_err | float | 1e-17 erg/s/cm^2 | Error in the flux | |||
| oiii_5007_inst_res | float | km/s | Instrumental resolution at the line center (measured for each spectrum from the ARC lamps) | |||
| oiii_5007_chisq | float | Reduced chi-squared of the line fit over the bandpass used for the EW measurement | ||||
| hei_5876_cont | float | 1e-17 erg/s/cm^2/AA | Continuum at line center from 200 pixel median smoothing of the emission-line subtracted continuum | |||
| hei_5876_cont_err | float | 1e-17 erg/s/cm^2/AA | Error in the continuum computed from the variance in the band pass | |||
| hei_5876_reqw | float | Ang | The equivalent width of the continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative). In this case the continuum comes from a running 200 pixel median and does not properly account for stellar absorption. In general the EQW measurements provide a better measure of the true equivalent width. The purpose of this measurement is to help characterize the stellar absorption effecting the line. (EW_stellar = REQW - EQW) | |||
| hei_5876_reqw_err | float | Ang | Error in the equivalent width described above | |||
| hei_5876_eqw | float | Ang | The equivalent width of the CB08 continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative) . This properly takes into account stellar absorption. Note that it will not be correct in the case of blended lines (ie NII & H-alpha) -- instead use FLUX/CONT. | |||
| hei_5876_eqw_err | float | Ang | Error in the equivalent width described above | |||
| hei_5876_flux | float | 1e-17 erg/s/cm^2 | Flux from Gaussian fit to continuum subtracted data. (Note that the fit is done simultaneously to all the lines so de-blending happens automatically) | |||
| hei_5876_flux_err | float | 1e-17 erg/s/cm^2 | Error in the flux | |||
| hei_5876_inst_res | float | km/s | Instrumental resolution at the line center (measured for each spectrum from the ARC lamps) | |||
| hei_5876_chisq | float | Reduced chi-squared of the line fit over the bandpass used for the EW measurement | ||||
| oi_6300_cont | float | 1e-17 erg/s/cm^2/AA | Continuum at line center from 200 pixel median smoothing of the emission-line subtracted continuum | |||
| oi_6300_cont_err | float | 1e-17 erg/s/cm^2/AA | Error in the continuum computed from the variance in the band pass | |||
| oi_6300_reqw | float | Ang | The equivalent width of the continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative). In this case the continuum comes from a running 200 pixel median and does not properly account for stellar absorption. In general the EQW measurements provide a better measure of the true equivalent width. The purpose of this measurement is to help characterize the stellar absorption effecting the line. (EW_stellar = REQW - EQW) | |||
| oi_6300_reqw_err | float | Ang | Error in the equivalent width described above | |||
| oi_6300_eqw | float | Ang | The equivalent width of the CB08 continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative) . This properly takes into account stellar absorption. Note that it will not be correct in the case of blended lines (ie NII & H-alpha) -- instead use FLUX/CONT. | |||
| oi_6300_eqw_err | float | Ang | Error in the equivalent width described above | |||
| oi_6300_flux | float | 1e-17 erg/s/cm^2 | Flux from Gaussian fit to continuum subtracted data. (Note that the fit is done simultaneously to all the lines so de-blending happens automatically) | |||
| oi_6300_flux_err | float | 1e-17 erg/s/cm^2 | Error in the flux | |||
| oi_6300_inst_res | float | km/s | Instrumental resolution at the line center (measured for each spectrum from the ARC lamps) | |||
| oi_6300_chisq | float | Reduced chi-squared of the line fit over the bandpass used for the EW measurement | ||||
| nii_6548_cont | float | 1e-17 erg/s/cm^2/AA | Continuum at line center from 200 pixel median smoothing of the emission-line subtracted continuum | |||
| nii_6548_cont_err | float | 1e-17 erg/s/cm^2/AA | Error in the continuum computed from the variance in the band pass | |||
| nii_6548_reqw | float | Ang | The equivalent width of the continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative). In this case the continuum comes from a running 200 pixel median and does not properly account for stellar absorption. In general the EQW measurements provide a better measure of the true equivalent width. The purpose of this measurement is to help characterize the stellar absorption effecting the line. (EW_stellar = REQW - EQW) | |||
| nii_6548_reqw_err | float | Ang | Error in the equivalent width described above | |||
| nii_6548_eqw | float | Ang | The equivalent width of the CB08 continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative) . This properly takes into account stellar absorption. Note that it will not be correct in the case of blended lines (ie NII & H-alpha) -- instead use FLUX/CONT. | |||
| nii_6548_eqw_err | float | Ang | Error in the equivalent width described above | |||
| nii_6548_flux | float | 1e-17 erg/s/cm^2 | Flux from Gaussian fit to continuum subtracted data. (Note that the fit is done simultaneously to all the lines so de-blending happens automatically) | |||
| nii_6548_flux_err | float | 1e-17 erg/s/cm^2 | Error in the flux | |||
| nii_6548_inst_res | float | km/s | Instrumental resolution at the line center (measured for each spectrum from the ARC lamps) | |||
| nii_6548_chisq | float | Reduced chi-squared of the line fit over the bandpass used for the EW measurement | ||||
| h_alpha_cont | float | 1e-17 erg/s/cm^2/AA | Continuum at line center from 200 pixel median smoothing of the emission-line subtracted continuum | |||
| h_alpha_cont_err | float | 1e-17 erg/s/cm^2/AA | Error in the continuum computed from the variance in the band pass | |||
| h_alpha_reqw | float | Ang | The equivalent width of the continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative). In this case the continuum comes from a running 200 pixel median and does not properly account for stellar absorption. In general the EQW measurements provide a better measure of the true equivalent width. The purpose of this measurement is to help characterize the stellar absorption effecting the line. (EW_stellar = REQW - EQW) | |||
| h_alpha_reqw_err | float | Ang | Error in the equivalent width described above | |||
| h_alpha_eqw | float | Ang | The equivalent width of the CB08 continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative) . This properly takes into account stellar absorption. Note that it will not be correct in the case of blended lines (ie NII & H-alpha) -- instead use FLUX/CONT. | |||
| h_alpha_eqw_err | float | Ang | Error in the equivalent width described above | |||
| h_alpha_flux | float | 1e-17 erg/s/cm^2 | Flux from Gaussian fit to continuum subtracted data. (Note that the fit is done simultaneously to all the lines so de-blending happens automatically) | |||
| h_alpha_flux_err | float | 1e-17 erg/s/cm^2 | Error in the flux | |||
| h_alpha_inst_res | float | km/s | Instrumental resolution at the line center (measured for each spectrum from the ARC lamps) | |||
| h_alpha_chisq | float | Reduced chi-squared of the line fit over the bandpass used for the EW measurement | ||||
| nii_6584_cont | float | 1e-17 erg/s/cm^2/AA | Continuum at line center from 200 pixel median smoothing of the emission-line subtracted continuum | |||
| nii_6584_cont_err | float | 1e-17 erg/s/cm^2/AA | Error in the continuum computed from the variance in the band pass | |||
| nii_6584_reqw | float | Ang | The equivalent width of the continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative). In this case the continuum comes from a running 200 pixel median and does not properly account for stellar absorption. In general the EQW measurements provide a better measure of the true equivalent width. The purpose of this measurement is to help characterize the stellar absorption effecting the line. (EW_stellar = REQW - EQW) | |||
| nii_6584_reqw_err | float | Ang | Error in the equivalent width described above | |||
| nii_6584_eqw | float | Ang | The equivalent width of the CB08 continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative) . This properly takes into account stellar absorption. Note that it will not be correct in the case of blended lines (ie NII & H-alpha) -- instead use FLUX/CONT. | |||
| nii_6584_eqw_err | float | Ang | Error in the equivalent width described above | |||
| nii_6584_flux | float | 1e-17 erg/s/cm^2 | Flux from Gaussian fit to continuum subtracted data. (Note that the fit is done simultaneously to all the lines so de-blending happens automatically) | |||
| nii_6584_flux_err | float | 1e-17 erg/s/cm^2 | Error in the flux | |||
| nii_6584_inst_res | float | km/s | Instrumental resolution at the line center (measured for each spectrum from the ARC lamps) | |||
| nii_6584_chisq | float | Reduced chi-squared of the line fit over the bandpass used for the EW measurement | ||||
| sii_6717_cont | float | 1e-17 erg/s/cm^2/AA | Continuum at line center from 200 pixel median smoothing of the emission-line subtracted continuum | |||
| sii_6717_cont_err | float | 1e-17 erg/s/cm^2/AA | Error in the continuum computed from the variance in the band pass | |||
| sii_6717_reqw | float | Ang | The equivalent width of the continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative). In this case the continuum comes from a running 200 pixel median and does not properly account for stellar absorption. In general the EQW measurements provide a better measure of the true equivalent width. The purpose of this measurement is to help characterize the stellar absorption effecting the line. (EW_stellar = REQW - EQW) | |||
| sii_6717_reqw_err | float | Ang | Error in the equivalent width described above | |||
| sii_6717_eqw | float | Ang | The equivalent width of the CB08 continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative) . This properly takes into account stellar absorption. Note that it will not be correct in the case of blended lines (ie NII & H-alpha) -- instead use FLUX/CONT. | |||
| sii_6717_eqw_err | float | Ang | Error in the equivalent width described above | |||
| sii_6717_flux | float | 1e-17 erg/s/cm^2 | Flux from Gaussian fit to continuum subtracted data. (Note that the fit is done simultaneously to all the lines so de-blending happens automatically) | |||
| sii_6717_flux_err | float | 1e-17 erg/s/cm^2 | Error in the flux | |||
| sii_6717_inst_res | float | km/s | Instrumental resolution at the line center (measured for each spectrum from the ARC lamps) | |||
| sii_6717_chisq | float | Reduced chi-squared of the line fit over the bandpass used for the EW measurement | ||||
| sii_6731_cont | float | 1e-17 erg/s/cm^2/AA | Continuum at line center from 200 pixel median smoothing of the emission-line subtracted continuum | |||
| sii_6731_cont_err | float | 1e-17 erg/s/cm^2/AA | Error in the continuum computed from the variance in the band pass | |||
| sii_6731_reqw | float | Ang | The equivalent width of the continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative). In this case the continuum comes from a running 200 pixel median and does not properly account for stellar absorption. In general the EQW measurements provide a better measure of the true equivalent width. The purpose of this measurement is to help characterize the stellar absorption effecting the line. (EW_stellar = REQW - EQW) | |||
| sii_6731_reqw_err | float | Ang | Error in the equivalent width described above | |||
| sii_6731_eqw | float | Ang | The equivalent width of the CB08 continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative) . This properly takes into account stellar absorption. Note that it will not be correct in the case of blended lines (ie NII & H-alpha) -- instead use FLUX/CONT. | |||
| sii_6731_eqw_err | float | Ang | Error in the equivalent width described above | |||
| sii_6731_flux | float | 1e-17 erg/s/cm^2 | Flux from Gaussian fit to continuum subtracted data. (Note that the fit is done simultaneously to all the lines so de-blending happens automatically) | |||
| sii_6731_flux_err | float | 1e-17 erg/s/cm^2 | Error in the flux | |||
| sii_6731_inst_res | float | km/s | Instrumental resolution at the line center (measured for each spectrum from the ARC lamps) | |||
| sii_6731_chisq | float | Reduced chi-squared of the line fit over the bandpass used for the EW measurement | ||||
| ariii7135_cont | float | 1e-17 erg/s/cm^2/AA | Continuum at line center from 200 pixel median smoothing of the emission-line subtracted continuum | |||
| ariii7135_cont_err | float | 1e-17 erg/s/cm^2/AA | Error in the continuum computed from the variance in the band pass | |||
| ariii7135_reqw | float | Ang | The equivalent width of the continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative). In this case the continuum comes from a running 200 pixel median and does not properly account for stellar absorption. In general the EQW measurements provide a better measure of the true equivalent width. The purpose of this measurement is to help characterize the stellar absorption effecting the line. (EW_stellar = REQW - EQW) | |||
| ariii7135_reqw_err | float | Ang | Error in the equivalent width described above | |||
| ariii7135_eqw | float | Ang | The equivalent width of the CB08 continuum-subtracted emission line computed from straight integration over the bandpasses listed below (emisison is negative) . This properly takes into account stellar absorption. Note that it will not be correct in the case of blended lines (ie NII & H-alpha) -- instead use FLUX/CONT. | |||
| ariii7135_eqw_err | float | Ang | Error in the equivalent width described above | |||
| ariii7135_flux | float | 1e-17 erg/s/cm^2 | Flux from Gaussian fit to continuum subtracted data. (Note that the fit is done simultaneously to all the lines so de-blending happens automatically) | |||
| ariii7135_flux_err | float | 1e-17 erg/s/cm^2 | Error in the flux | |||
| ariii7135_inst_res | float | km/s | Instrumental resolution at the line center (measured for each spectrum from the ARC lamps) | |||
| ariii7135_chisq | float | Reduced chi-squared of the line fit over the bandpass used for the EW measurement | ||||
| oii_sigma | float | km/s | The width of the [O II] line in a free fit (ie. not tied to other emission lines) | |||
| oii_flux | float | 1e-17 erg/s/cm^2 | The flux of the [O II] doublet from a free fit. | |||
| oii_flux_err | float | 1e-17 erg/s/cm^2 | The estimated uncertainty on OII_FLUX | |||
| oii_voff | float | km/s | The velocity offset of the [O II] doublet from a free fit | |||
| oii_chi2 | float | chi^2 of the fit to the [O II] line in free fit | ||||
| oiii_sigma | float | km/s | The width of the [O III]5007 line in a free fit (ie. not tied to other emission lines) | |||
| oiii_flux | float | 1e-17 erg/s/cm^2 | The flux of the [O III]5007 line from a free fit. | |||
| oiii_flux_err | float | 1e-17 erg/s/cm^2 | The estimated uncertainty on OIII_FLUX | |||
| oiii_voff | float | km/s | The velocity offset of the [O III]5007 line from a free fit | |||
| oiii_chi2 | float | chi^2 of the fit to the [O III]5007 line in free fit | ||||
| spectofiber | float | The multiplicative scale factor applied to the original flux and error spectra prior to measurement of the emission lines to improve the spectrophotometric accuracy. The rescaling insures that a synthetic r-band magnitude computed from the spectrum matches the r-band fiber magnitude measured by the photometric pipeline. |
All PhotoObj pairs within 0.5 arcmin
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| objID | long | The unique objId of the center object | ||||
| neighborObjID | long | The objId of the neighbor | ||||
| distance | double | arcmins | Distance between center and neighbor | |||
| type | int | Object type of the center | ||||
| neighborType | int | Object type of the neighbor | ||||
| mode | int | object is primary, secondary, family, outside | ||||
| neighborMode | int | is neighbor primary, secondary, family, outside |
Map PhotoObj which are potential targets to sector
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| objID | long | ID of the best PhotoObj | ||||
| regionID | long | ID of the sector | ||||
| status | int | Status of the object in the survey | ||||
| primTarget | int | Bit mask of primary target categories the object was selected in. | ||||
| secTarget | int | Bit mask of secondary target categories the object was selected in. | ||||
| petroMag_r | float | mag | Petrosian flux | |||
| extinction_r | float | mag | Extinction in each filter |
Half-spaces (caps) describing the SDSS imaging geometr
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| sdssPolygonID | int | integer description of polygon | ||||
| x | double | x-component of normal vector | ||||
| y | double | y-component of normal vector | ||||
| z | double | z-component of normal vector | ||||
| c | double | offset from center along normal | ||||
| xMangle | double | mangle version of x-component | ||||
| yMangle | double | mangle version of y-component | ||||
| zMangle | double | mangle version of z-component | ||||
| cMangle | double | mangle version of offset from center | ||||
| loadVersion | int | Load Version |
Matched list of polygons and field
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| sdssPolygonID | int | integer designator of polygon | ||||
| fieldID | long | field identification | ||||
| loadVersion | int | Load Version |
Polygons describing SDSS imaging data window functio
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| sdssPolygonID | int | integer description of polygon | ||||
| nField | int | number of fields in the polygon | ||||
| primaryFieldID | long | ID of primary field in this polygon | ||||
| ra | double | deg | RA (J2000 deg) in approximate center of polygon | |||
| dec | double | deg | Dec (J2000 deg) in approximate center of polygon | |||
| area | double | square deg | area of polygon | |||
| loadVersion | int | Load Version |
Stores the information about set of unique Sector region
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| regionID | long | unique, sequential ID | ||||
| nTiles | int | number of overlapping tiles | ||||
| tiles | string | list of tiles in Sector | ||||
| targetVersion | string | the version of target selection ran over the sector -/K ID_VERSION | ||||
| area | float | deg^2 | area of this overlap region |
Match tiles to sectors, wedges adn sectorlets, and vice versa
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| regionID | long | ID of the sector | ||||
| type | string | type of the sector | ||||
| tile | int | tile number | ||||
| isMask | int | flag that shows sign of tile (1 is negative) |
Contains the parameters used for a version of the target selection cod
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| targetVersion | string | version of target selection software | ||||
| paramFile | string | version of target selection software | ||||
| name | string | parameter name | ||||
| value | string | value used for the parameter |
Contains information about each individual tile on the sky
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| tile | int | (unique) tile number | ||||
| tileRun | int | run of the tiling software | ||||
| raCen | double | deg | right ascension of tile center | |||
| decCen | double | deg | declination of the tile center | |||
| htmID | long | htm tree info | ||||
| cx | double | x projection of vector on unit sphere | ||||
| cy | double | y projection of vector on unit sphere | ||||
| cz | double | z projection of vector on unit sphere | ||||
| untiled | int | 1: this tile later "untiled," releasing targets to be assigned to another tile, 0: otherwise | ||||
| nTargets | int | number of targets assigned to this tile | ||||
| loadVersion | int | Load Version |
Information on all targets run through tiling for SDSS-I and SDSS-I
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| targetID | long | Unique SDSS identifier composed from [skyVersion=0,rerun,run,camcol,field,obj]. | ||||
| run | int | Drift scan run number for targeting | ||||
| rerun | int | Reprocessing number for targeting | ||||
| camcol | int | Camera column number for targeting | ||||
| field | int | Field number for targeting | ||||
| obj | int | Object id number for targeting | ||||
| ra | double | deg | right ascension | |||
| dec | double | deg | declination | |||
| htmID | long | htm tree info | ||||
| cx | double | x projection of vector on unit sphere | ||||
| cy | double | y projection of vector on unit sphere | ||||
| cz | double | z projection of vector on unit sphere | ||||
| primTarget | int | primary target bitmask | ||||
| secTarget | int | secondary target bitmask | ||||
| tiPriority | int | tiling priority level (lower means higher priority) | ||||
| tileAll | int | First tile number this object was assigned to | ||||
| tiMaskAll | int | Combined value of tiling results bitmask | ||||
| collisionGroupAll | int | unique ID of collisionGroup | ||||
| photoObjID | long | hashed ID of photometric object in best version of the sky | ||||
| specObjID | long | hashed ID of spectroscopic object in best version of the sky | ||||
| regionID | int | ID of tiling region, 0 if unset | ||||
| loadVersion | int | Load Version |
Information about boundary and mask regions in SDSS-I and SDSS-I
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| tilingGeometryID | int | unique identifier for this tilingRegion | ||||
| tileRun | int | run of tiling software | ||||
| stripe | int | stripe containing the boundary | ||||
| nsbx | string | b: official stripe boundaries should be included, x: use the full rectangle | ||||
| isMask | int | 1: tiling mask, 0: tiling boundary | ||||
| coordType | int | specifies coordinate system for the boundaries | ||||
| lambdamu_0 | double | deg | first lower bound | |||
| lambdamu_1 | double | deg | first upper bound | |||
| etanu_0 | double | deg | second lower bound | |||
| etanu_1 | double | deg | second upper bound | |||
| lambdaLimit_0 | double | deg | minimum survey latitude for this stripe for region in which primaries are selected (-9999 if no limit) | |||
| lambdaLimit_1 | double | deg | maximum survey latitude for this stripe for region in which primaries are selected (-9999 if no limit) | |||
| targetVersion | string | version of target software within this boundary | ||||
| firstArea | double | deg^2 | area of sky covered by this boundary that was not covered by previous boundaries | |||
| loadVersion | int | Load Version |
Results of individual tiling runs for each tiled targe
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| targetID | long | Unique SDSS identifier composed from [skyVersion=0,rerun,run,camcol,field,obj]. | ||||
| tileRun | int | Run of tiling software | ||||
| tid | int | Unique ID of objects within tiling run | ||||
| tiMask | int | Value of tiling results bitmask for this run | ||||
| collisionGroup | int | unique ID of collisionGroup in this tiling run | ||||
| tile | int | Tile this object was assigned to in this run | ||||
| loadVersion | int | Load Version |
Contains basic information for a run of tiling Contains basic information for a run of tilin
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| tileRun | int | (unique) tiling run number | ||||
| ctileVersion | string | version of ctile software | ||||
| tilepId | string | unique id for tiling run | ||||
| programName | string | character string of program | ||||
| primTargetMask | int | bit mask for target types to be tiled | ||||
| secTargetMask | int | bit mask for target types to be tiled | ||||
| loadVersion | int | Load Version |
SEGUE-1 and SEGUE-2 target selection run on all imaging dat
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| objid | long | unique id, points to photoObj | ||||
| segue1_target1 | int | SEGUE-1 primary target selection flag | ||||
| segue1_target2 | int | SEGUE-1 secondary target selection flag | ||||
| segue2_target1 | int | SEGUE-2 primary target selection flag | ||||
| segue2_target2 | int | SEGUE-2 secondary target selection flag | ||||
| lcolor | float | mag | SEGUE-1 and -2 target selection color: -0.436*uMag+1.129*gMag-0.119*rMag-0.574*iMag+0.1984 (Lenz et al.1998) | |||
| scolor | float | mag | SEGUE-1 target selection color: -0.249*uMag+0.794*gMag-0.555*rMag+0.234+0.011*p1s-0.010 (Helmi et al. 2003) | |||
| p1s | float | mag | SEGUE-1 target selection color: 0.91*umg+0.415*umg-1.280 (Helmi et al. 2003) | |||
| totalpm | float | mas/year | sqrt(PMRA*PMRA+PMDEC*PMDEC), in mas/year | |||
| hg | float | mag | reduced proper motion, gMag+5*log10(TOTALPM/1000)+5 | |||
| Mi | float | mag | 4.471+7.907*imz-0.837*imz*imz used in SEGUE-1 target selection, unused in SEGUE-2 | |||
| disti | float | mag | 10^((iMag-Mi+5)/5.0) used in SEGUE-1 target selection, unused in SEGUE-2 | |||
| Hr | float | mag | reduced pm (uncorr r): PSFMAG_r+5*log10(TOTALPM/1000)+5 | |||
| vmi_trans1 | float | mag | V-I from VMAG_TRANS-(iMag-0.337*rmi-0.37) | |||
| vmi_trans2 | float | mag | V-I from 0.877*gmr+0.358 | |||
| vmag_trans | float | mag | V mag from gMag - 0.587*gmr -0.011 | |||
| Mv_trans | float | mag | ||||
| distv_kpc | float | kpc | 10^(dmV/5.-2.) where VMAG_TRANS-(3.37*VMI_TRANS1+2.89) | |||
| vtrans_galrest | float | km/s | transvere velocity, km/s, derived from TOTALPM and DISTV_KPC, in a frame at rest w.r.t the Galaxy | |||
| mutrans_galradrest | float | mas/year | derived PM (mas/year) perpendicular to the Galactocentric radial vector, assuming all motion is along a Galactocentric radial vector, in a frame at rest w.r.t the Galaxy | |||
| murad_galradrest | float | mas/year | derived PM (mas/year) along the Galactocentric radial vector, assuming all motion is along a Galactocentric radial vector, in a frame at rest w.r.t the Galaxy | |||
| vtot_galradrest | float | km/s | total velocity, km/s, derived from TOTALPM and DISTV_KPC, in a frame at rest w.r.t the Galaxy | |||
| mg_tohv | float | mag | 5.7 + 10.0*(GMR - 0.375) | |||
| vtrans_tohv | float | km/s | transverse velocity in Galactocentric coords, using the distance estimate from MG_TOHV which is appropriate for old stars near the MSTO and corrected for peculiar solar motion 16.6 km/s toward RA,Dec 267.5,28.1 | |||
| pm1sigma_tohv | float | mas/year | Estimate of the 1-sigma error in total proper motion at this r magnitude. Formula is sqrt(4.56*4.56 + frate*2.30*2.30), where frate is 10^(0.4*(rMag-19.5)). The constants come from the Munn et al. 2004 (AJ, 127, 3034) paper describing the recalibration of USNOB with SDSS. | |||
| v1sigmaerr_tohv | float | km/s | The corresponding 1-sigma error in the transverse velocity based on PM1SIGMA_TOHV and the the distance estimate using MG_TOHV |
Contains outputs from the SEGUE Stellar Parameter Pipeline (SSPP)
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| SPECOBJID | long | id number | ||||
| bestObjID | long | Object ID of photoObj match (flux-based) | ||||
| TARGETOBJID | long | targeted object ID | ||||
| sciencePrimary | int | Best version of spectrum at this location (defines default view SpecObj) | ||||
| legacyPrimary | int | Best version of spectrum at this location, among Legacy plates | ||||
| seguePrimary | int | Best version of spectrum at this location, among SEGUE plates (defines default view SpecObj) | ||||
| PLATE | long | Plate number | ||||
| MJD | long | Modified Julian Date | ||||
| FIBER | long | Fiber ID | ||||
| RUN2D | string | Name of 2D rerun | ||||
| RUN1D | string | Name of 1D rerun | ||||
| RUNSSPP | string | Name of SSPP rerun | ||||
| H83side | float | Angstrom | Hzeta line index from local continuum at 3889.0 with band widths of 3.0 | |||
| H83cont | float | Angstrom | Hzeta line index from global continuum at 3889.0 with band widths of 3.0 | |||
| H83err | float | Angstrom | Hzeta line index error in the lind band at 3889.0 with band widths of 3.0 | |||
| H83mask | int | Hzeta pixel quality check, =0 good, =1 bad at 3889.0 with band widths of 3.0 | ||||
| H812side | float | Angstrom | Hzeta line index from local continuum at 3889.1 with band widths of 12.0 | |||
| H812cont | float | Angstrom | Hzeta line index from global continuum at 3889.1 with band widths of 12.0 | |||
| H812err | float | Angstrom | Hzeta line index error in the lind band at 3889.1 with band widths of 12.0 | |||
| H812mask | int | Hzeta pixel quality check, =0 good, =1 bad at 3889.1 with band widths of 12.0 | ||||
| H824side | float | Angstrom | Hzeta line index from local continuum at 3889.1 with band widths of 24.0 | |||
| H824cont | float | Angstrom | Hzeta line index from global continuum at 3889.1 with band widths of 24.0 | |||
| H824err | float | Angstrom | Hzeta line index error in the lind band at 3889.1 with band widths of 24.0 | |||
| H824mask | int | Hzeta pixel quality check, =0 good, =1 bad at 3889.1 with band widths of 24.0 | ||||
| H848side | float | Angstrom | Hzeta line index from local continuum at 3889.1 with band widths of 48.0 | |||
| H848cont | float | Angstrom | Hzeta line index from global continuum at 3889.1 with band widths of 48.0 | |||
| H848err | float | Angstrom | Hzeta line index error in the lind band at 3889.1 with band widths of 48.0 | |||
| H848mask | int | Hzeta pixel quality check, =0 good, =1 bad at 3889.1 with band widths of 48.0 | ||||
| KP12side | float | Angstrom | Ca II K line index from local continuum at 3933.7 with band widths of 12.0 | |||
| KP12cont | float | Angstrom | Ca II K line index from global continuum at 3933.7 with band widths of 12.0 | |||
| KP12err | float | Angstrom | Ca II K line index error in the lind band at 3933.7 with band widths of 12.0 | |||
| KP12mask | int | Ca II K pixel quality check, =0 good, =1 bad at 3933.7 with band widths of 12.0 | ||||
| KP18side | float | Angstrom | Ca II K line index from local continuum at 3933.7 with band widths of 18.0 | |||
| KP18cont | float | Angstrom | Ca II K line index from global continuum at 3933.7 with band widths of 18.0 | |||
| KP18err | float | Angstrom | Ca II K line index error in the lind band at 3933.7 with band widths of 18.0 | |||
| KP18mask | int | Ca II K pixel quality check =0, good, =1 bad at 3933.7 with band widths of 18.0 | ||||
| KP6side | float | Angstrom | Ca II K line index from local continuum at 3933.7 with band widths of 6.0 | |||
| KP6cont | float | Angstrom | Ca II K line index from global continuum at 3933.7 with band widths of 6.0 | |||
| KP6err | float | Angstrom | Ca II K line index error in the lind band at 3933.7 with band widths of 6.0 | |||
| KP6mask | int | Ca II K pixel quality check =0, good, =1 bad at 3933.7 with band widths of 6.0 | ||||
| CaIIKside | float | Angstrom | Ca II K line index from local continuum at 3933.6 with band widths of 30.0 | |||
| CaIIKcont | float | Angstrom | Ca II K line index from global continuum at 3933.6 with band widths of 30.0 | |||
| CaIIKerr | float | Angstrom | Ca II K line index error in the lind band at 3933.6 with band widths of 30.0 | |||
| CaIIKmask | int | Ca II K pixel quality check =0, good, =1 bad at 3933.6 with band widths of 30.0 | ||||
| CaIIHKside | float | Angstrom | Ca II H and K line index from local continuum at 3962.0 with band widths of 75.0 | |||
| CaIIHKcont | float | Angstrom | Ca II H and K line index from global continuum at 3962.0 with band widths of 75.0 | |||
| CaIIHKerr | float | Angstrom | Ca II H and K line index error in the lind band at 3962.0 with band widths of 75.0 | |||
| CaIIHKmask | int | Ca II H and K pixel quality check =0, good, =1 bad at 3962.0 with band widths of 75.0 | ||||
| Hepsside | float | Angstrom | Hepsilon line index from local continuum at 3970.0 with band widths of 50.0 | |||
| Hepscont | float | Angstrom | Hepsilon line index from global continuum at 3970.0 with band widths of 50.0 | |||
| Hepserr | float | Angstrom | Hepsilon line index error in the lind band at 3970.0 with band widths of 50.0 | |||
| Hepsmask | int | Hepsilon pixel quality check =0, good, =1 bad at 3970.0 with band widths of 50.0 | ||||
| KP16side | float | Angstrom | Ca II K line index from local continuum at 3933.7 with band widths of 16.0 | |||
| KP16cont | float | Angstrom | Ca II K line index from global continuum at 3933.7 with band widths of 16.0 | |||
| KP16err | float | Angstrom | Ca II K line index error in the lind band at 3933.7 with band widths of 16.0 | |||
| KP16mask | int | Ca II K pixel quality check =0, good, =1 bad at 3933.7 with band widths of 16.0 | ||||
| SrII1side | float | Angstrom | Sr II line index from local continuum at 4077.0 with band widths of 8.0 | |||
| SrII1cont | float | Angstrom | Sr II line index from global continuum at 4077.0 with band widths of 8.0 | |||
| SrII1err | float | Angstrom | Sr II line index error in the lind band at 4077.0 with band widths of 8.0 | |||
| SrII1mask | int | Sr II pixel quality check =0, good, =1 bad at 4077.0 with band widths of 8.0 | ||||
| HeI121side | float | Angstrom | He I line index from local continuum at 4026.2 with band widths of 12.0 | |||
| HeI121cont | float | Angstrom | He I line index from global continuum at 4026.2 with band widths of 12.0 | |||
| HeI121err | float | Angstrom | He I line index error in the lind band at 4026.2 with band widths of 12.0 | |||
| HeI121mask | int | He I pixel quality check =0, good, =1 bad at 4026.2 with band widths of 12.0 | ||||
| Hdelta12side | float | Angstrom | Hdelta line index from local continuum at 4101.8 with band widths of 12.0 | |||
| Hdelta12cont | float | Angstrom | Hdelta line index from global continuum at 4101.8 with band widths of 12.0 | |||
| Hdelta12err | float | Angstrom | Hdelta line index error in the lind band at 4101.8 with band widths of 12.0 | |||
| Hdelta12mask | int | Hdelta pixel quality check =0, good, =1 bad at 4101.8 with band widths of 12.0 | ||||
| Hdelta24side | float | Angstrom | Hdelta line index from local continuum at 4101.8 with band widths of 24.0 | |||
| Hdelta24cont | float | Angstrom | Hdelta line index from global continuum at 4101.8 with band widths of 24.0 | |||
| Hdelta24err | float | Angstrom | Hdelta line index error in the lind band at 4101.8 with band widths of 24.0 | |||
| Hdelta24mask | int | Hdelta pixel quality check =0, good, =1 bad at 4101.8 with band widths of 24.0 | ||||
| Hdelta48side | float | Angstrom | Hdelta line index from local continuum at 4101.8 with band widths of 48.0 | |||
| Hdelta48cont | float | Angstrom | Hdelta line index from global continuum at 4101.8 with band widths of 48.0 | |||
| Hdelta48err | float | Angstrom | Hdelta line index error in the lind band at 4101.8 with band widths of 48.0 | |||
| Hdelta48mask | int | Hdelta pixel quality check =0, good, =1 bad at 4101.8 with band widths of 48.0 | ||||
| Hdeltaside | float | Angstrom | Hdelta line index from local continuum at 4102.0 with band widths of 64.0 | |||
| Hdeltacont | float | Angstrom | Hdelta line index from global continuum at 4102.0 with band widths of 64.0 | |||
| Hdeltaerr | float | Angstrom | Hdelta line index error in the lind band at 4102.0 with band widths of 64.0 | |||
| Hdeltamask | int | Hdelta pixel quality check =0, good, =1 bad at 4102.0 with band widths of 64.0 | ||||
| CaI4side | float | Angstrom | Ca I line index from local continuum at 4226.0 with band widths of 4.0 | |||
| CaI4cont | float | Angstrom | Ca I line index from global continuum at 4226.0 with band widths of 4.0 | |||
| CaI4err | float | Angstrom | Ca I line index error in the lind band at 4226.0 with band widths of 4.0 | |||
| CaI4mask | int | Ca I pixel quality check =0, good, =1 bad at 4226.0 with band widths of 4.0 | ||||
| CaI12side | float | Angstrom | Ca I line index from local continuum at 4226.7 with band widths of 12.0 | |||
| CaI12cont | float | Angstrom | Ca I line index from global continuum at 4226.7 with band widths of 12.0 | |||
| CaI12err | float | Angstrom | Ca I line index error in the lind band at 4226.7 with band widths of 12.0 | |||
| CaI12mask | int | Ca I pixel quality check =0, good, =1 bad at 4226.7 with band widths of 12.0 | ||||
| CaI24side | float | Angstrom | Ca I line index from local continuum at 4226.7 with band widths of 24.0 | |||
| CaI24cont | float | Angstrom | Ca I line index from global continuum at 4226.7 with band widths of 24.0 | |||
| CaI24err | float | Angstrom | Ca I line index error in the lind band at 4226.7 with band widths of 24.0 | |||
| CaI24mask | int | Ca I pixel quality check =0, good, =1 bad at 4226.7 with band widths of 24.0 | ||||
| CaI6side | float | Angstrom | Ca I line index from local continuum at 4226.7 with band widths of 6.0 | |||
| CaI6cont | float | Angstrom | Ca I line index from global continuum at 4226.7 with band widths of 6.0 | |||
| CaI6err | float | Angstrom | Ca I line index error in the lind band at 4226.7 with band widths of 6.0 | |||
| CaI6mask | int | Ca I pixel quality check =0, good, =1 bad at 4226.7 with band widths of 6.0 | ||||
| Gside | float | Angstrom | G band line index from local continuum at 4305.0 with band widths of 15.0 | |||
| Gcont | float | Angstrom | G band line index from global continuum at 4305.0 with band widths of 15.0 | |||
| Gerr | float | Angstrom | G band line index error in the lind band at 4305.0 with band widths of 15.0 | |||
| Gmask | int | G band pixel quality check =0, good, =1 bad at 4305.0 with band widths of 15.0 | ||||
| Hgamma12side | float | Angstrom | Hgamma line index from local continuum at 4340.5 with band widths of 12.0 | |||
| Hgamma12cont | float | Angstrom | Hgamma line index from global continuum at 4340.5 with band widths of 12.0 | |||
| Hgamma12err | float | Angstrom | Hgamma line index error in the lind band at 4340.5 with band widths of 12.0 | |||
| Hgamma12mask | int | Hgamma pixel quality check =0, good, =1 bad at 4340.5 with band widths of 12.0 | ||||
| Hgamma24side | float | Angstrom | Hgamma line index from local continuum at 4340.5 with band widths of 24.0 | |||
| Hgamma24cont | float | Angstrom | Hgamma line index from global continuum at 4340.5 with band widths of 24.0 | |||
| Hgamma24err | float | Angstrom | Hgamma line index error in the lind band at 4340.5 with band widths of 24.0 | |||
| Hgamma24mask | int | Hgamma pixel quality check =0, good, =1 bad at 4340.5 with band widths of 24.0 | ||||
| Hgamma48side | float | Angstrom | Hgamma line index from local continuum at 4340.5 with band widths of 48.0 | |||
| Hgamma48cont | float | Angstrom | Hgamma line index from global continuum at 4340.5 with band widths of 48.0 | |||
| Hgamma48err | float | Angstrom | Hgamma line index error in the lind band at 4340.5 with band widths of 48.0 | |||
| Hgamma48mask | int | Hgamma pixel quality check =0, good, =1 bad at 4340.5 with band widths of 48.0 | ||||
| Hgammaside | float | Angstrom | Hgamma line index from local continuum at 4340.5 with band widths of 54.0 | |||
| Hgammacont | float | Angstrom | Hgamma line index from global continuum at 4340.5 with band widths of 54.0 | |||
| Hgammaerr | float | Angstrom | Hgamma line index error in the lind band at 4340.5 with band widths of 54.0 | |||
| Hgammamask | int | Hgamma pixel quality check =0, good, =1 bad at 4340.5 with band widths of 54.0 | ||||
| HeI122side | float | Angstrom | He I line index from local continuum at 4471.7 with band widths of 12.0 | |||
| HeI122cont | float | Angstrom | He I line index from global continuum at 4471.7 with band widths of 12.0 | |||
| HeI122err | float | Angstrom | He I line index error in the lind band at 4471.7 with band widths of 12.0 | |||
| HeI122mask | int | He I pixel quality check =0, good, =1 bad at 4471.7 with band widths of 12.0 | ||||
| Gblueside | float | Angstrom | G band line index from local continuum at 4305.0 with band widths of 26.0 | |||
| Gbluecont | float | Angstrom | G band line index from global continuum at 4305.0 with band widths of 26.0 | |||
| Gblueerr | float | Angstrom | G band line index error in the lind band at 4305.0 with band widths of 26.0 | |||
| Gbluemask | int | G band pixel quality check =0, good, =1 bad at 4305.0 with band widths of 26.0 | ||||
| Gwholeside | float | Angstrom | G band line index from local continuum at 4321.0 with band widths of 28.0 | |||
| Gwholecont | float | Angstrom | G band line index from global continuum at 4321.0 with band widths of 28.0 | |||
| Gwholeerr | float | Angstrom | G band line index error in the lind band at 4321.0 with band widths of 28.0 | |||
| Gwholemask | int | G band pixel quality check =0, good, =1 bad at 4321.0 with band widths of 28.0 | ||||
| Baside | float | Angstrom | Ba line index from local continuum at 4554.0 with band widths of 6.0 | |||
| Bacont | float | Angstrom | Ba line index from global continuum at 4554.0 with band widths of 6.0 | |||
| Baerr | float | Angstrom | Ba line index error in the lind band at 4554.0 with band widths of 6.0 | |||
| Bamask | int | Ba pixel quality check =0, good, =1 bad at 4554.0 with band widths of 6.0 | ||||
| C12C13side | float | Angstrom | C12C13 band line index from local continuum at 4737.0 with band widths of 36.0 | |||
| C12C13cont | float | Angstrom | C12C13 band line index from global continuum at 4737.0 with band widths of 36.0 | |||
| C12C13err | float | Angstrom | C12C13 band line index error in the lind band at 4737.0 with band widths of 36.0 | |||
| C12C13mask | int | C12C13 band pixel quality check =0, good, =1 bad at 4737.0 with band widths of 36.0 | ||||
| CC12side | float | Angstrom | C2 band line index from local continuum at 4618.0 with band widths of 256.0 | |||
| CC12cont | float | Angstrom | C2 band line index from global continuum at 4618.0 with band widths of 256.0 | |||
| CC12err | float | Angstrom | C2 band line index error in the lind band at 4618.0 with band widths of 256.0 | |||
| CC12mask | int | C2 band pixel quality check =0, good, =1 bad at 4618.0 with band widths of 256.0 | ||||
| metal1side | float | Angstrom | Metallic line index from local continuum at 4584.0 with band widths of 442.0 | |||
| metal1cont | float | Angstrom | Metallic line index from global continuum at 4584.0 with band widths of 442.0 | |||
| metal1err | float | Angstrom | Metlllic line index error in the lind band at 4584.0 with band widths of 442.0 | |||
| metal1mask | int | Metal1ic pixel quality check =0, good, =1 bad at 4584.0 with band widths of 442.0 | ||||
| Hbeta12side | float | Angstrom | Hbeta line index from local continuum at 4862.3 with band widths of 12.0 | |||
| Hbeta12cont | float | Angstrom | Hbeta line index from global continuum at 4862.3 with band widths of 12.0 | |||
| Hbeta12err | float | Angstrom | Hbeta line index error in the lind band at 4862.3 with band widths of 12.0 | |||
| Hbeta12mask | int | Hbeta pixel quality check =0, good, =1 bad at 4862.3 with band widths of 12.0 | ||||
| Hbeta24side | float | Angstrom | Hbeta line index from local continuum at 4862.3 with band widths of 24.0 | |||
| Hbeta24cont | float | Angstrom | Hbeta line index from global continuum at 4862.3 with band widths of 24.0 | |||
| Hbeta24err | float | Angstrom | Hbeta line index error in the lind band at 4862.3 with band widths of 24.0 | |||
| Hbeta24mask | int | Hbeta pixel quality check =0, good, =1 bad at 4862.3 with band widths of 24.0 | ||||
| Hbeta48side | float | Angstrom | Hbeta line index from local continuum at 4862.3 with band widths of 48.0 | |||
| Hbeta48cont | float | Angstrom | Hbeta line index from global continuum at 4862.3 with band widths of 48.0 | |||
| Hbeta48err | float | Angstrom | Hbeta line index error in the lind band at 4862.3 with band widths of 48.0 | |||
| Hbeta48mask | int | Hbeta pixel quality check =0, good, =1 bad at 4862.3 with band widths of 48.0 | ||||
| Hbetaside | float | Angstrom | Hbeta line index from local continuum at 4862.3 with band widths of 60.0 | |||
| Hbetacont | float | Angstrom | Hbeta line index from global continuum at 4862.3 with band widths of 60.0 | |||
| Hbetaerr | float | Angstrom | Hbeta line index error in the lind band at 4862.3 with band widths of 60.0 | |||
| Hbetamask | int | Hbeta pixel quality check =0, good, =1 bad at 4862.3 with band widths of 60.0 | ||||
| C2side | float | Angstrom | C2 band line index from local continuum at 5052.0 with band widths of 204.0 | |||
| C2cont | float | Angstrom | C2 band line index from global continuum at 5052.0 with band widths of 204.0 | |||
| C2err | float | Angstrom | C2 band line index error in the lind band at 5052.0 with band widths of 204.0 | |||
| C2mask | int | C2 band pixel quality check =0, good, =1 bad at 5052.0 with band widths of 204.0 | ||||
| C2MgIside | float | Angstrom | C2 and Mg I line index from local continuum at 5069.0 with band widths of 238.0 | |||
| C2MgIcont | float | Angstrom | C2 and Mg I line index from global continuum at 5069.0 with band widths of 238.0 | |||
| C2MgIerr | float | Angstrom | C2 and Mg I line index error in the lind band at 5069.0 with band widths of 238.0 | |||
| C2MgImask | int | C2 and Mg I pixel quality check =0, good, =1 bad at 5069.0 with band widths of 238.0 | ||||
| MgHMgIC2side | float | Angstrom | MgH, Mg I, and C2 line index from local continuum at 5085.0 with band widths of 270.0 | |||
| MgHMgIC2cont | float | Angstrom | MgH, Mg I, and C2 line index from global continuum at 5085.0 with band widths of 270.0 | |||
| MgHMgIC2err | float | Angstrom | MgH, Mg I, and C2 line index error in the lind band at 5085.0 with band widths of 270.0 | |||
| MgHMgIC2mask | int | MgH, Mg I, and C2 pixel quality check =0, good, =1 bad at 5085.0 with band widths of 270.0 | ||||
| MgHMgIside | float | Angstrom | MgH and Mg I line index from local continuum at 5198.0 with band widths of 44.0 | |||
| MgHMgIcont | float | Angstrom | MgH and Mg I line index from global continuum at 5198.0 with band widths of 44.0 | |||
| MgHMgIerr | float | Angstrom | MgH and Mg I line index error in the lind band at 5198.0 with band widths of 44.0 | |||
| MgHMgImask | int | MgH_MgI pixel quality check =0, good, =1 bad at 5198.0 with band widths of 44.0 | ||||
| MgHside | float | Angstrom | MgH line index from local continuum at 5210.0 with band widths of 20.0 | |||
| MgHcont | float | Angstrom | MgH line index from global continuum at 5210.0 with band widths of 20.0 | |||
| MgHerr | float | Angstrom | MgH line index error in the lind band at 5210.0 with band widths of 20.0 | |||
| MgHmask | int | MgH pixel quality check =0, good, =1 bad at 5210.0 with band widths of 20.0 | ||||
| CrIside | float | Angstrom | Cr I line index from local continuum at 5206.0 with band widths of 12.0 | |||
| CrIcont | float | Angstrom | Cr I line index from global continuum at 5206.0 with band widths of 12.0 | |||
| CrIerr | float | Angstrom | Cr I line index error in the lind band at 5206.0 with band widths of 12.0 | |||
| CrImask | int | Cr I pixel quality check =0, good, =1 bad at 5206.0 with band widths of 12.0 | ||||
| MgIFeIIside | float | Angstrom | Mg I and Fe II line index from local continuum at 5175.0 with band widths of 20.0 | |||
| MgIFeIIcont | float | Angstrom | Mg I and Fe II line index from global continuum at 5175.0 with band widths of 20.0 | |||
| MgIFeIIerr | float | Angstrom | Mg I and Fe II line index error in the lind band at 5175.0 with band widths of 20.0 | |||
| MgIFeIImask | int | Mg I and Fe II pixel quality check =0, good, =1 bad at 5175.0 with band widths of 20.0 | ||||
| MgI2side | float | Angstrom | Mg I line index from local continuum at 5183.0 with band widths of 2.0 | |||
| MgI2cont | float | Angstrom | Mg I line index from global continuum at 5183.0 with band widths of 2.0 | |||
| MgI2err | float | Angstrom | Mg I line index error in the lind band at 5183.0 with band widths of 2.0 | |||
| MgI2mask | int | Mg I pixel quality check =0, good, =1 bad at 5183.0 with band widths of 2.0 | ||||
| MgI121side | float | Angstrom | Mg I line index from local continuum at 5170.5 with band widths of 12.0 | |||
| MgI121cont | float | Angstrom | Mg I line index from global continuum at 5170.5 with band widths of 12.0 | |||
| MgI121err | float | Angstrom | Mg I line index error in the lind band at 5170.5 with band widths of 12.0 | |||
| MgI121mask | int | Mg I pixel quality check =0, good, =1 bad at 5170.5 with band widths of 12.0 | ||||
| MgI24side | float | Angstrom | Mg I line index from local continuum at 5176.5 with band widths of 24.0 | |||
| MgI24cont | float | Angstrom | Mg I line index from global continuum at 5176.5 with band widths of 24.0 | |||
| MgI24err | float | Angstrom | Mg I line index error in the lind band at 5176.5 with band widths of 24.0 | |||
| MgI24mask | int | Mg I pixel quality check =0, good, =1 bad at 5176.5 with band widths of 24.0 | ||||
| MgI122side | float | Angstrom | Mg I line index from local continuum at 5183.5 with band widths of 12.0 | |||
| MgI122cont | float | Angstrom | Mg I line index from global continuum at 5183.5 with band widths of 12.0 | |||
| MgI122err | float | Angstrom | Mg I line index error in the lind band at 5183.5 with band widths of 12.0 | |||
| MgI122mask | int | Mg I pixel quality check =0, good, =1 bad at 5183.5 with band widths of 12.0 | ||||
| NaI20side | float | Angstrom | Na I line index from local continuum at 5890.0 with band widths of 20.0 | |||
| NaI20cont | float | Angstrom | Na I line index from global continuum at 5890.0 with band widths of 20.0 | |||
| NaI20err | float | Angstrom | Na I line index error in the lind band at 5890.0 with band widths of 20.0 | |||
| NaI20mask | int | Na I pixel quality check =0, good, =1 bad at 5890.0 with band widths of 20.0 | ||||
| Na12side | float | Angstrom | Na line index from local continuum at 5892.9 with band widths of 12.0 | |||
| Na12cont | float | Angstrom | Na line index from global continuum at 5892.9 with band widths of 12.0 | |||
| Na12err | float | Angstrom | Na line index error in the lind band at 5892.9 with band widths of 12.0 | |||
| Na12mask | int | Na pixel quality check =0, good, =1 bad at 5892.9 with band widths of 12.0 | ||||
| Na24side | float | Angstrom | Na line index from local continuum at 5892.9 with band widths of 24.0 | |||
| Na24cont | float | Angstrom | Na line index from global continuum at 5892.9 with band widths of 24.0 | |||
| Na24err | float | Angstrom | Na line index error in the lind band at 5892.9 with band widths of 24.0 | |||
| Na24mask | int | Na pixel quality check =0, good, =1 bad at 5892.9 with band widths of 24.0 | ||||
| Halpha12side | float | Angstrom | Halpha line index from local continuum at 6562.8 with band widths of 12.0 | |||
| Halpha12cont | float | Angstrom | Halpha line index from global continuum at 6562.8 with band widths of 12.0 | |||
| Halpha12err | float | Angstrom | Halpha line index error in the lind band at 6562.8 with band widths of 12.0 | |||
| Halpha12mask | int | Halpha pixel quality check =0, good, =1 bad at 6562.8 with band widths of 12.0 | ||||
| Halpha24side | float | Angstrom | Halpha line index from local continuum at 6562.8 with band widths of 24.0 | |||
| Halpha24cont | float | Angstrom | Halpha line index from global continuum at 6562.8 with band widths of 24.0 | |||
| Halpha24err | float | Angstrom | Halpha line index error in the lind band at 6562.8 with band widths of 24.0 | |||
| Halpha24mask | int | Halpha pixel quality check =0, good, =1 bad at 6562.8 with band widths of 24.0 | ||||
| Halpha48side | float | Angstrom | Halpha line index from local continuum at 6562.8 with band widths of 48.0 | |||
| Halpha48cont | float | Angstrom | Halpha line index from global continuum at 6562.8 with band widths of 48.0 | |||
| Halpha48err | float | Angstrom | Halpha line index error in the lind band at 6562.8 with band widths of 48.0 | |||
| Halpha48mask | int | Halpha pixel quality check =0, good, =1 bad at 6562.8 with band widths of 48.0 | ||||
| Halpha70side | float | Angstrom | Halpha line index from local continuum at 6562.8 with band widths of 70.0 | |||
| Halpha70cont | float | Angstrom | Halpha line index from global continuum at 6562.8 with band widths of 70.0 | |||
| Halpha70err | float | Angstrom | Halpha line index error in the lind band at 6562.8 with band widths of 70.0 | |||
| Halpha70mask | int | Halpha pixel quality check =0, good, =1 bad at 6562.8 with band widths of 70.0 | ||||
| CaHside | float | Angstrom | CaH line index from local continuum at 6788.0 with band widths of 505.0 | |||
| CaHcont | float | Angstrom | CaH line index from global continuum at 6788.0 with band widths of 505.0 | |||
| CaHerr | float | Angstrom | CaH line index error in the lind band at 6788.0 with band widths of 505.0 | |||
| CaHmask | int | CaH pixel quality check =0, good, =1 bad at 6788.0 with band widths of 505.0 | ||||
| TiOside | float | Angstrom | TiO line index from local continuum at 7209.0 with band widths of 333.3 | |||
| TiOcont | float | Angstrom | TiO line index from global continuum at 7209.0 with band widths of 333.3 | |||
| TiOerr | float | Angstrom | TiO line index error in the lind band at 7209.0 with band widths of 333.3 | |||
| TiOmask | int | TiO pixel quality check =0, good, =1 bad at 7209.0 with band widths of 333.3 | ||||
| CNside | float | Angstrom | CN line index from local continuum at 6890.0 with band widths of 26.0 | |||
| CNcont | float | Angstrom | CN line index from global continuum at 6890.0 with band widths of 26.0 | |||
| CNerr | float | Angstrom | CN line index error in the lind band at 6890.0 with band widths of 26.0 | |||
| CNmask | int | CN pixel quality check =0, good, =1 bad at 6890.0 with band widths of 26.0 | ||||
| OItripside | float | Angstrom | O I triplet line index from local continuu at 7775.0 with band widths of 30.0 | |||
| OItripcont | float | Angstrom | O I triplet line index from global continuum at 7775.0 with band widths of 30.0 | |||
| OItriperr | float | Angstrom | O I triplet line index error in the lind band at 7775.0 with band widths of 30.0 | |||
| OItripmask | int | O I triplet pixel quality check =0, good, =1 bad at 7775.0 with band widths of 30.0 | ||||
| KI34side | float | Angstrom | K I line index from local continuum at 7687.0 with band widths of 34.0 | |||
| KI34cont | float | Angstrom | K I line index from global continuum at 7687.0 with band widths of 34.0 | |||
| KI34err | float | Angstrom | K I line index error in the lind band at 7687.0 with band widths of 34.0 | |||
| KI34mask | int | K I pixel quality check =0, good, =1 bad at 7687.0 with band widths of 34.0 | ||||
| KI95side | float | Angstrom | K I line index from local continuum at 7688.0 with band widths of 95.0 | |||
| KI95cont | float | Angstrom | K I line index from global continuum at 7688.0 with band widths of 95.0 | |||
| KI95err | float | Angstrom | K I line index error in the lind band at 7688.0 with band widths of 95.0 | |||
| KI95mask | int | K I pixel quality check =0, good, =1 bad at 7688.0 with band widths of 95.0 | ||||
| NaI15side | float | Angstrom | Na I line index from local continuum at 8187.5 with band widths of 15.0 | |||
| NaI15cont | float | Angstrom | Na I line index from global continuum at 8187.5 with band widths of 15.0 | |||
| NaI15err | float | Angstrom | Na I line index error in the lind band at 8187.5 with band widths of 15.0 | |||
| NaI15mask | int | Na I pixel quality check =0, good, =1 bad at 8187.5 with band widths of 15.0 | ||||
| NaIredside | float | Angstrom | Na I line index from local continuum at 8190.2 with band widths of 33.0 | |||
| NaIredcont | float | Angstrom | Na I line index from global continuum at 8190.2 with band widths of 33.0 | |||
| NaIrederr | float | Angstrom | Na I line index error in the lind band at 8190.2 with band widths of 33.0 | |||
| NaIredmask | int | Na I pixel quality check =0, good, =1 bad at 8190.2 with band widths of 33.0 | ||||
| CaII26side | float | Angstrom | Ca II triplet line index from local continuum at 8498.0 with band widths of 26.0 | |||
| CaII26cont | float | Angstrom | Ca II triplet line index from global continuum at 8498.0 with band widths of 26.0 | |||
| CaII26err | float | Angstrom | Ca II triplet line index error in the lind band at 8498.0 with band widths of 26.0 | |||
| CaII26mask | int | Ca II triplet pixel quality check =0, good, =1 bad at 8498.0 with band widths of 26.0 | ||||
| Paschen13side | float | Angstrom | Paschen line index from local continuum at 8467.5 with band widths of 13.0 | |||
| Paschen13cont | float | Angstrom | Paschen line index from global continuum at 8467.5 with band widths of 13.0 | |||
| Paschen13err | float | Angstrom | Paschen line index error in the lind band at 8467.5 with band widths of 13.0 | |||
| Paschen13mask | int | Paschen pixel quality check =0, good, =1 bad at 8467.5 with band widths of 13.0 | ||||
| CaII29side | float | Angstrom | Ca II triplet line index from local continuum at 8498.5 with band widths of 29.0 | |||
| CaII29cont | float | Angstrom | Ca II triplet line index from global continuum at 8498.5 with band widths of 29.0 | |||
| CaII29err | float | Angstrom | Ca II triplet line index error in the lind band at 8498.5 with band widths of 29.0 | |||
| CaII29mask | int | Ca II triplet pixel quality check =0, good, =1 bad at 8498.5 with band widths of 29.0 | ||||
| CaII401side | float | Angstrom | Ca II triplet line index from local continuum at 8542.0 with band widths of 40.0 | |||
| CaII401cont | float | Angstrom | Ca II triplet line index from global continuum at 8542.0 with band widths of 40.0 | |||
| CaII401err | float | Angstrom | Ca II triplet line index error in the lind band at 8542.0 with band widths of 40.0 | |||
| CaII401mask | int | Ca II triplet pixel quality check =0, good, =1 bad at 8542.0 with band widths of 40.0 | ||||
| CaII161side | float | Angstrom | Ca II triplet_1 line index from local continuum at 8542.0 with band widths of 16.0 | |||
| CaII161cont | float | Angstrom | Ca II triplet_1 line index from global continuum at 8542.0 with band widths of 16.0 | |||
| CaII161err | float | Angstrom | Ca II triplet_1 line index error in the lind band at 8542.0 with band widths of 16.0 | |||
| CaII161mask | int | Ca II triplet_1 pixel quality check =0, good, =1 bad at 8542.0 with band widths of 16.0 | ||||
| Paschen421side | float | Angstrom | Paschen line index from local continuum at 8598.0 with band widths of 42.0 | |||
| Paschen421cont | float | Angstrom | Paschen line index from global continuum at 8598.0 with band widths of 42.0 | |||
| Paschen421err | float | Angstrom | Paschen line index error in the lind band at 8598.0 with band widths of 42.0 | |||
| Paschen421mask | int | Paschen pixel quality check =0, good, =1 bad at 8598.0 with band widths of 42.0 | ||||
| CaII162side | float | Angstrom | Ca II triplet line index from local continuum at 8662.1 with band widths of 16.0 | |||
| CaII162cont | float | Angstrom | Ca II triplet line index from global continuum at 8662.1 with band widths of 16.0 | |||
| CaII162err | float | Angstrom | Ca II triplet line index error in the lind band at 8662.1 with band widths of 16.0 | |||
| CaII162mask | int | Ca II triplet pixel quality check =0, good, =1 bad at 8662.1 with band widths of 16.0 | ||||
| CaII402side | float | Angstrom | Ca II triplet line index from local continuum at 8662.0 with band widths of 40.0 | |||
| CaII402cont | float | Angstrom | Ca II triplet line index from global continuum at 8662.0 with band widths of 40.0 | |||
| CaII402err | float | Angstrom | Ca II triplet line index error in the lind band at 8662.0 with band widths of 40.0 | |||
| CaII402mask | int | Ca II triplet pixel quality check =0, good, =1 bad at 8662.0 with band widths of 40.0 | ||||
| Paschen422side | float | Angstrom | Paschen line index from local continuum at 8751.0 with band widths of 42.0 | |||
| Paschen422cont | float | Angstrom | Paschen line index from global continuum at 8751.0 with band widths of 42.0 | |||
| Paschen422err | float | Angstrom | Paschen line index error in the lind band at 8751.0 with band widths of 42.0 | |||
| Paschen422mask | int | Paschen pixel quality check =0, good, =1 bad at 8751.0 with band widths of 42.0 | ||||
| TiO5side | float | TiO5 line index from local continuum at 7134.4 with band widths of 5.0 | ||||
| TiO5cont | float | TiO5 line index from global continuum at 7134.4 with band widths of 5.0 | ||||
| TiO5err | float | TiO5 line index error in the lind band at 7134.4 with band widths of 5.0 | ||||
| TiO5mask | int | TiO5 pixel quality check =0, good, =1 bad at 7134.4 with band widths of 5.0 | ||||
| TiO8side | float | TiO8 line index from local continuum at 8457.3 with band widths of 30.0 | ||||
| TiO8cont | float | TiO8 line index from global continuum at 8457.3 with band widths of 30.0 | ||||
| TiO8err | float | TiO8 line index error in the lind band at 8457.3 with band widths of 30.0 | ||||
| TiO8mask | int | TiO8 pixel quality check =0, good, =1 bad at 8457.3 with band widths of 30.0 | ||||
| CaH1side | float | CaH1 line index from local continuum at 6386.7 with band widths of 10.0 | ||||
| CaH1cont | float | CaH1 line index from global continuum at 6386.7 with band widths of 10.0 | ||||
| CaH1err | float | CaH1 line index error in the lind band at 6386.7 with band widths of 10.0 | ||||
| CaH1mask | int | CaH1 pixel quality check =0, good, =1 bad at 6386.7 with band widths of 10.0 | ||||
| CaH2side | float | CaH2 line index from local continuum at 6831.9 with band widths of 32.0 | ||||
| CaH2cont | float | CaH2 line index from global continuum at 6831.9 with band widths of 32.0 | ||||
| CaH2err | float | CaH2 line index error in the lind band at 6831.9 with band widths of 32.0 | ||||
| CaH2mask | int | CaH2 pixel quality check =0, good, =1 bad at 6831.9 with band widths of 32.0 | ||||
| CaH3side | float | CaH3 line index from local continuum at 6976.9 with band widths of 30.0 | ||||
| CaH3cont | float | CaH3 line index from global continuum at 6976.9 with band widths of 30.0 | ||||
| CaH3err | float | CaH3 line index error in the lind band at 6976.9 with band widths of 30.0 | ||||
| CaH3mask | int | CaH3 pixel quality check =0, good, =1 bad at 6976.9 with band widths of 30.0 | ||||
| UVCNside | float | CN line index at 3839 | ||||
| UVCNcont | float | CN line index at 3839 | ||||
| UVCNerr | float | CN line index error at 3829 | ||||
| UVCNmask | int | CN pixel quality check =0, good, =1 bad at 3839 | ||||
| BLCNside | float | CN line index at 4142 | ||||
| BLCNcont | float | CN line index at 4142 | ||||
| BLCNerr | float | CN line index error at 4142 | ||||
| BLCNmask | int | CN pixel quality check =0, good, =1 bad at 4142 | ||||
| FEI1side | float | Angstrom | Fe I line index at 4045.8 with band widths of 2.5 | |||
| FEI1cont | float | Angstrom | Fe I line index at 4045.8 with band widths of 2.5 | |||
| FEI1err | float | Angstrom | Fe I line index error at 4045.8 with band widths of 2.5 | |||
| FEI1mask | int | Fe I pixel quality check =0, good, =1 bad at 4045.8 with band widths of 2.5 | ||||
| FEI2side | float | Angstrom | Fe I line index at 4063.6 with band widths of 2.0 | |||
| FEI2cont | float | Angstrom | Fe I line index at 4063.6 with band widths of 2.0 | |||
| FEI2err | float | Angstrom | Fe I line index error at 4063.6 with band widths of 2.0 | |||
| FEI2mask | int | Fe I pixel quality check =0, good, =1 bad at 4063.6 with band widths of 2.0 | ||||
| FEI3side | float | Angstrom | Fe I line index at 4071.7 with band widths of 2.0 | |||
| FEI3cont | float | Angstrom | Fe I line index at 4071.7 with band widths of 2.0 | |||
| FEI3err | float | Angstrom | Fe I line index error at 4071.7 with band widths of 2.0 | |||
| FEI3mask | int | Fe I pixel quality check =0, good, =1 bad at 4071.7 with band widths of 2.0 | ||||
| SRII2side | float | Angstrom | Sr II line index at 4077.7 with band widths of 2.0 | |||
| SRII2cont | float | Angstrom | Sr II line index at 4077.7 with band widths of 2.0 | |||
| SRII2err | float | Angstrom | Sr II line index error at 4077.7 with band widths of 2.0 | |||
| SRII2mask | int | Sr II pixel quality check =0, good, =1 bad at 4077.7 with band widths of 2.0 | ||||
| FEI4side | float | Fe I line index at 4679.5 with band widths of 87.0 | ||||
| FEI4cont | float | Fe I line index at 4679.5 with band widths of 87.0 | ||||
| FEI4err | float | Fe I line index error at 4679.5 with band widths of 87.0 | ||||
| FEI4mask | int | Fe I pixel quality check =0, good, =1 bad at 4679.5 with band widths of 87.0 | ||||
| FEI5side | float | Fe I line index at 5267.4 with band widths of 38.8 | ||||
| FEI5cont | float | Fe I line index at 5267.4 with band widths of 38.8 | ||||
| FEI5err | float | Fe I line index error at 5267.4 with band widths of 38.8 | ||||
| FEI5mask | int | Fe I pixel quality check =0, good, =1 bad at 5267.4 with band widths of 38.8 |
Contains outputs from the SEGUE Stellar Parameter Pipeline (SSPP)
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| SPECOBJID | long | id number, match in specObjAll | ||||
| BESTOBJID | long | Object ID of best PhotoObj match (flux-based) | ||||
| FLUXOBJID | long | Object ID of best PhotoObj match (position-based) | ||||
| TARGETOBJID | long | targeted object ID | ||||
| PLATEID | long | Database ID of Plate (match in plateX) | ||||
| sciencePrimary | int | Best version of spectrum at this location (defines default view SpecObj) | ||||
| legacyPrimary | int | Best version of spectrum at this location, among Legacy plates | ||||
| seguePrimary | int | Best version of spectrum at this location, among SEGUE plates (defines default view SpecObj) | ||||
| FIRSTRELEASE | string | Name of first release this object was associated with | ||||
| SURVEY | string | Survey name | ||||
| PROGRAMNAME | string | Program name | ||||
| CHUNK | string | Chunk name | ||||
| PLATERUN | string | Plate drill run name | ||||
| MJD | long | Modified Julian Date of observation | ||||
| PLATE | long | Plate number | ||||
| FIBERID | long | Fiber number (1-640) | ||||
| RUN2D | string | Name of 2D rerun | ||||
| RUN1D | string | Name of 1D rerun | ||||
| RUNSSPP | string | Name of SSPP rerun | ||||
| TARGETSTRING | string | ASCII translation of target selection information as determined at the time the plate was designed | ||||
| PRIMTARGET | long | Target selection information at plate design, primary science selection (for backwards compatibility) | ||||
| SECTARGET | long | Target selection information at plate design, secondary/qa/calib selection (for backwards compatibility) | ||||
| LEGACY_TARGET1 | long | Legacy target selection information at plate design, primary science selection | ||||
| LEGACY_TARGET2 | long | Legacy target selection information at plate design, secondary/qa/calib selection | ||||
| SPECIAL_TARGET1 | long | Special program target selection information at plate design, primary science selection | ||||
| SPECIAL_TARGET2 | long | Special program target selection information at plate design, secondary/qa/calib selection | ||||
| SEGUE1_TARGET1 | long | SEGUE-1 target selection information at plate design, primary science selection | ||||
| SEGUE1_TARGET2 | long | SEGUE-1 target selection information at plate design, secondary/qa/calib selection | ||||
| SEGUE2_TARGET1 | long | SEGUE-2 target selection information at plate design, primary science selection | ||||
| SEGUE2_TARGET2 | long | SEGUE-2 target selection information at plate design, secondary/qa/calib selection | ||||
| SPECTYPEHAMMER | string | Spectral Type from HAMMER | ||||
| SPECTYPESUBCLASS | string | SpecBS sub-classification | ||||
| FLAG | string | Flag with combination of four letters among BCdDEgGhHlnNSV, n=normal | ||||
| TEFFADOP | float | Kelvin | Adopted Teff, bi-weigth average of estimators with indicator variable of 1 | |||
| TEFFADOPN | int | Kelvin | Number of estimators used in bi-weight average | |||
| TEFFADOPUNC | float | Kelvin | Error in the adopted temperature | |||
| TEFFHA24 | float | Kelvin | Teff estimate from HA24 | |||
| TEFFHD24 | float | Kelvin | Teff estimate from HD24 | |||
| TEFFNGS1 | float | Kelvin | Teff estimate from NGS1 | |||
| TEFFANNSR | float | Kelvin | Teff estimate from ANNSR | |||
| TEFFANNRR | float | Kelvin | Teff estimate from ANNRR | |||
| TEFFWBG | float | Kelvin | Teff estimate from WBG | |||
| TEFFK24 | float | Kelvin | Teff estimate from k24 | |||
| TEFFKI13 | float | Kelvin | Teff estimate from ki13 | |||
| TEFFHA24IND | int | Indicator variable, = 0 bad, = 1 good | ||||
| TEFFHD24IND | int | Indicator variable, = 0 bad, = 1 good | ||||
| TEFFNGS1IND | int | Indicator variable, = 0 bad, = 1 good | ||||
| TEFFANNSRIND | int | Indicator variable, = 0 bad, = 1 good | ||||
| TEFFANNRRIND | int | Indicator variable, = 0 bad, = 1 good | ||||
| TEFFWBGIND | int | Indicator variable, = 0 bad, = 1 good | ||||
| TEFFK24IND | int | Indicator variable, = 0 bad, = 1 good | ||||
| TEFFKI13IND | int | Indicator variable, = 0 bad, = 1 good | ||||
| TEFFHA24UNC | float | Kelvin | Error in Teff estimate from HA24 | |||
| TEFFHD24UNC | float | Kelvin | Error in Teff estimate from HD24 | |||
| TEFFNGS1UNC | float | Kelvin | Error in Teff estimate from NGS1 | |||
| TEFFANNSRUNC | float | Kelvin | Error in Teff estimate from ANNSR | |||
| TEFFANNRRUNC | float | Kelvin | Error in Teff estimate from ANNRR | |||
| TEFFWBGUNC | float | Kelvin | Error in Teff estimate from WBG | |||
| TEFFK24UNC | float | Kelvin | Error in Teff estimate from k24 | |||
| TEFFKI13UNC | float | Kelvin | Error in Teff estimate from ki13 | |||
| LOGGADOP | float | dex | Adopted log g, bi-weigth average of estimators with indicator variable of 2 | |||
| LOGGADOPN | int | Number of log g estimators in used bi-weight average | ||||
| LOGGADOPUNC | float | dex | Error in the adopted log g | |||
| LOGGNGS2 | float | dex | log g estimate from NGS2 | |||
| LOGGNGS1 | float | dex | log g estimate from NGS1 | |||
| LOGGANNSR | float | dex | log g estimate from ANNSR | |||
| LOGGANNRR | float | dex | log g estimate from ANNRR | |||
| LOGGCAI1 | float | dex | log g estimate from CaI1 | |||
| LOGGWBG | float | dex | log g estimate from WBG | |||
| LOGGK24 | float | dex | log g estimate from k24 | |||
| LOGGKI13 | float | dex | log g estimate from ki13 | |||
| LOGGNGS2IND | int | Indicator variable, = 0 bad, = 1 good | ||||
| LOGGNGS1IND | int | Indicator variable, = 0 bad, = 1 good | ||||
| LOGGANNSRIND | int | Indicator variable, = 0 bad, = 1 good | ||||
| LOGGANNRRIND | int | Indicator variable, = 0 bad, = 1 good | ||||
| LOGGCAI1IND | int | Indicator variable, = 0 bad, = 1 good | ||||
| LOGGWBGIND | int | Indicator variable, = 0 bad, = 1 good | ||||
| LOGGK24IND | int | Indicator variable, = 0 bad, = 1 good | ||||
| LOGGKI13IND | int | Indicator variable, = 0 bad, = 1 good | ||||
| LOGGNGS2UNC | float | dex | Error in log g estimate from NGS2 | |||
| LOGGNGS1UNC | float | dex | Error in log g estimate from NGS1 | |||
| LOGGANNSRUNC | float | dex | Error in log g estimate from ANNSR | |||
| LOGGANNRRUNC | float | dex | Error in log g estimate from ANNRR | |||
| LOGGCAI1UNC | float | dex | Error in log g estimate from CaI1 | |||
| LOGGWBGUNC | float | dex | Error in log g estimate from WBG | |||
| LOGGK24UNC | float | dex | Error in log g estimate from k24 | |||
| LOGGKI13UNC | float | dex | Error in log g estimate from ki13 | |||
| FEHADOP | float | dex | Adopted [Fe/H], bi-weigth average of estimators with indicator variable of 2 | |||
| FEHADOPN | int | Number of estimators used in bi-weight average | ||||
| FEHADOPUNC | float | dex | Error in the adopted [Fe/H] | |||
| FEHNGS2 | float | dex | [Fe/H] estimate from NGS2 | |||
| FEHNGS1 | float | dex | [Fe/H] estimate from NGS1 | |||
| FEHANNSR | float | dex | [Fe/H] estimate from ANNSR | |||
| FEHANNRR | float | dex | [Fe/H] estimate from ANNRR | |||
| FEHCAIIK1 | float | dex | [Fe/H] estimate from CaIIK1 | |||
| FEHCAIIK2 | float | dex | [Fe/H] estimate from CaIIK2 | |||
| FEHCAIIK3 | float | dex | [Fe/H] estimate from CaIIK3 | |||
| FEHWBG | float | dex | [Fe/H] estimate from WBG | |||
| FEHK24 | float | dex | [Fe/H] estimate from k24 | |||
| FEHKI13 | float | dex | [Fe/H] estimate from ki13 | |||
| FEHNGS2IND | int | Indicator variable, = 0 bad, = 1 low S/N or out of g-r color range, = 2 good | ||||
| FEHNGS1IND | int | Indicator variable, = 0 bad, = 1 low S/N or out of g-r color range, = 2 good | ||||
| FEHANNSRIND | int | Indicator variable, = 0 bad, = 1 low S/N or out of g-r color range, = 2 good | ||||
| FEHANNRRIND | int | Indicator variable, = 0 bad, = 1 low S/N or out of g-r color range, = 2 good | ||||
| FEHCAIIK1IND | int | Indicator variable, = 0 bad, = 1 low S/N or out of g-r color range, = 2 good | ||||
| FEHCAIIK2IND | int | Indicator variable, = 0 bad, = 1 low S/N or out of g-r color range, = 2 good | ||||
| FEHCAIIK3IND | int | Indicator variable, = 0 bad, = 1 low S/N or out of g-r color range, = 2 good | ||||
| FEHWBGIND | int | Indicator variable, = 0 bad, = 1 low S/N or out of g-r color range, = 2 good | ||||
| FEHK24IND | int | Indicator variable, = 0 bad, = 1 low S/N or out of g-r color range, = 2 good | ||||
| FEHKI13IND | int | Indicator variable, = 0 bad, = 1 low S/N or out of g-r color range, = 2 good | ||||
| FEHNGS2UNC | float | dex | Error in [Fe/H] estimate from NGS2 | |||
| FEHNGS1UNC | float | dex | Error in [Fe/H] estimate from NGS1 | |||
| FEHANNSRUNC | float | dex | Error in [Fe/H] estimate from ANNSR | |||
| FEHANNRRUNC | float | dex | Error in [Fe/H] estimate from ANNRR | |||
| FEHCAIIK1UNC | float | dex | Error in [Fe/H] estiimate from CaIIK1 | |||
| FEHCAIIK2UNC | float | dex | Error in [Fe/H] estimate from CaIIK2 | |||
| FEHCAIIK3UNC | float | dex | Error in [Fe/H] estimate from CaIIK3 | |||
| FEHWBGUNC | float | dex | Error in [Fe/H] estimate from WBG | |||
| FEHK24UNC | float | dex | Error in [Fe/H] estimate from k24 | |||
| FEHKI13UNC | float | dex | Error in [Fe/H] estimate from ki13 | |||
| SNR | float | Average S/N per pixel over 4000 - 8000 A | ||||
| QA | int | Quality check on spectrum, depending on S/N | ||||
| CCCAHK | float | Correlation coefficient over 3850-4250 A | ||||
| CCMGH | float | Correlation coefficient over 4500-5500 A | ||||
| TEFFSPEC | float | Kelvin | Spectroscopically determined Teff, color independent | |||
| TEFFSPECN | int | Number of estimators used in average | ||||
| TEFFSPECUNC | float | Kelvin | Error in the spectroscopically determined Teff | |||
| LOGGSPEC | float | dex | Spectroscopically determined log g, color independent | |||
| LOGGSPECN | int | Number of estimators used in average | ||||
| LOGGSPECUNC | float | dex | Error in the spectroscopically determined log g | |||
| FEHSPEC | float | dex | Spectroscopically determined [Fe/H], color independent | |||
| FEHSPECN | int | Number of estimators used in average | ||||
| FEHSPECUNC | float | dex | Error in the spectroscopically determined [Fe/H] | |||
| ACF1 | float | Auto-Correlation Function over 4000-4086/4116-4325/4355-4500 | ||||
| ACF1SNR | float | Average signal-to-noise ratio in Auto-Correlation Function 1 (ACF1) | ||||
| ACF2 | float | Auto-Correlation Functioin over 4000-4086/4116-4280/4280-4500 | ||||
| ACF2SNR | float | Average signal-to-noise ratio in Auto-Correlation Function 2 (ACF2) | ||||
| INSPECT | string | Flag with combination of six letters among FTtMmCn, for inspecting spectra | ||||
| ELODIERVFINAL | float | km/s | Velocity as measured by Elodie library templates, converted to km/s and with the empirical 7.3 km/s offset applied (see Yanny et al. 2009, AJ, 137, 4377) | |||
| ELODIERVFINALERR | float | km/s | Uncertainty in the measured Elodie RV, as determined from the chisq template-fitting routine. See the discussion of empirically-determined velocity errors in Yanny et al. 2009, AJ, 137, 4377 | |||
| ZWARNING | long | Warning flags about velocity/redshift determinations | ||||
| TEFFIRFM | float | Kelvin | Teff from Infrared Flux Methods (IRFM) | |||
| TEFFIRFMIND | int | Indicator variable, = 0 bad, = 1 good | ||||
| TEFFIRFMUNC | float | dex | Error in Teff estimate from IRFM | |||
| LOGGNGS1IRFM | float | dex | log g estimate from NGS1 while fixing Teff from IRFM | |||
| LOGGNGS1IRFMIND | int | Indicator variable, = 0 bad, =1 good | ||||
| LOGGNGS1IRFMUNC | float | dex | Error in log g from NGS1 while fixing Teff from IRFM | |||
| FEHNGS1IRFM | float | dex | [Fe/H] estimate from NGS1 while fixing Teff from IRFM | |||
| FEHNGS1IRFMIND | int | Indicator variable, =0 bad, = 1 good | ||||
| FEHNGS1IRFMUNC | float | dex | Error in [Fe/H] from NGS1 while fixing Teff from IRFM | |||
| LOGGCAI1IRFM | float | dex | log g estimate from CAI1 with fixed IRFM Teff | |||
| LOGGCAI1IRFMIND | int | Indicator variable, =0 bad, = 1 good | ||||
| LOGGCAI1IRFMUNC | float | dex | Error in log g from CAI1 with fixed IRFM Teff | |||
| FEHCAIIK1IRFM | float | dex | [Fe/H] from CaIIK1 with fixed IRFM Teff | |||
| FEHCAIIK1IRFMIND | int | Indicator variable, =0 bad, = 1 good | ||||
| FEHCAIIK1IRFMUNC | float | dex | Error in [Fe/H] from CaIIK1 with fixed IRFM Teff |
Derived quantities calculated by the SEGUE-2 target selection pipeline
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| OBJID | long | Object ID matching DR8 | ||||
| RUN | long | Run number | ||||
| RERUN | long | Rerun number | ||||
| CAMCOL | long | Camera column number | ||||
| FIELD | long | Field number | ||||
| OBJ | long | Object | ||||
| RA | double | degree | RA | |||
| DEC | double | degree | Dec | |||
| L | double | degree | Galactic longitude | |||
| B | double | degree | Galactic latitude | |||
| FIBERMAG_u | float | mag | u band fiber magnitudue | |||
| FIBERMAG_g | float | mag | g band fiber magnitudue | |||
| FIBERMAG_r | float | mag | r band fiber magnitudue | |||
| FIBERMAG_i | float | mag | i band fiber magnitudue | |||
| FIBERMAG_z | float | mag | z band fiber magnitudue | |||
| PSFMAG_u | float | mag | u band PSF magnitude | |||
| PSFMAG_g | float | mag | g band PSF magnitude | |||
| PSFMAG_r | float | mag | r band PSF magnitude | |||
| PSFMAG_i | float | mag | i band PSF magnitude | |||
| PSFMAG_z | float | mag | z band PSF magnitude | |||
| EXTINCTION_u | float | mag | u band extinction | |||
| EXTINCTION_g | float | mag | g band extinction | |||
| EXTINCTION_r | float | mag | r band extinction | |||
| EXTINCTION_i | float | mag | i band extinction | |||
| EXTINCTION_z | float | mag | z band extinction | |||
| ROWC | int | pix | row centroid | |||
| COLC | int | pix | column centroid | |||
| TYPE | int | object type from photometric reductions | ||||
| FLAGS | long | combined flags from all bands | ||||
| FLAGS_u | long | u band flag | ||||
| FLAGS_g | long | g band flag | ||||
| FLAGS_r | long | r band flag | ||||
| FLAGS_i | long | i band flag | ||||
| FLAGS_z | long | z band flag | ||||
| PSFMAGERR_u | float | mag | Error in u band PSF magnitude | |||
| PSFMAGERR_g | float | mag | Error in u band PSF magnitude | |||
| PSFMAGERR_r | float | mag | Error in u band PSF magnitude | |||
| PSFMAGERR_i | float | mag | Error in u band PSF magnitude | |||
| PSFMAGERR_z | float | mag | Error in u band PSF magnitude | |||
| PLATEID | long | Hash of plate and MJD | ||||
| SPECOBJID | long | Spectroscopic object ID | ||||
| PLATE | long | Plate number | ||||
| MJD | long | Modified Julian Date | ||||
| FIBERID | long | Fiber number | ||||
| ORIGINALPLATEID | long | Original plate ID hash (if targeted based on previous spectrum) | ||||
| ORIGINALSPECOBJID | long | Original spectroscopic object ID (if targeted based on previous spectrum) | ||||
| ORIGINALPLATE | long | Original plate number (if targeted based on previous spectrum) | ||||
| ORIGINALMJD | long | Original Modified Julian Date (if targeted based on previous spectrum) | ||||
| ORIGINALFIBERID | long | Original fiber number (if targeted based on previous spectrum)(if targeted based on previous spectrum) | ||||
| BESTOBJID | long | Best object ID | ||||
| TARGETOBJID | long | Target object ID | ||||
| PRIMTARGET | int | Primary target | ||||
| SECTARGET | int | Secondary target | ||||
| SEGUE1_TARGET1 | long | SEGUE-1 target selection information at plate design, primary science selection | ||||
| SEGUE1_TARGET2 | long | SEGUE-1 target selection information at plate design, secondary/qa/calib selection | ||||
| SEGUE2_TARGET1 | int | bitmask that records the category or categories for which this object passed the selection criteria | ||||
| SEGUE2_TARGET2 | int | bitmask that records the category or categories of "standards" for the pipeline, special calibration targets like Stetson standards or globular cluster stars, for which this object passed the selection criteria | ||||
| MATCH | long | ?? | ||||
| DELTA | double | ?? | ||||
| PML | double | mas/year? | Proper motion in Galactic longitude? | |||
| PMB | double | mas/year? | Proper motion in Galactic latitude? | |||
| PMRA | double | mas/year? | Proper motion in RA | |||
| PMDEC | double | mas/year? | Proper motion in DEC | |||
| PMRAERR | double | mas/year? | Proper motion error in RA | |||
| PMDECERR | double | mas/year? | Proper motion error in DEC | |||
| PMSIGRA | double | mas/year? | ||||
| PMSIGDEC | double | mas/year? | ||||
| NFIT | int | |||||
| DIST22 | double | |||||
| DIST20 | double | |||||
| uMAG0 | float | mag | u extinction-corrected (SFD 98) psf magnitude | |||
| gMAG0 | float | mag | g extinction-corrected (SFD 98) psf magnitude | |||
| rMAG0 | float | mag | r extinction-corrected (SFD 98) psf magnitude | |||
| iMAG0 | float | mag | i extinction-corrected (SFD 98) psf magnitude | |||
| zMAG0 | float | mag | z extinction-corrected (SFD 98) psf magnitude | |||
| umg0 | float | mag | u-g, extinction corrected magnitudes | |||
| gmr0 | float | mag | g-r, extinction corrected magnitudes | |||
| rmi0 | float | mag | r-i, extinction corrected magnitudes | |||
| imz0 | float | mag | i-z, extinction corrected magnitudes | |||
| gmi0 | float | mag | g-i, extinction corrected magnitudes | |||
| umgERR | float | mag | PSFMAGERR_u and PSFMAGERR_g added in quadrature | |||
| gmrERR | float | mag | PSFMAGERR_g and PSFMAGERR_r added in quadrature | |||
| rmiERR | float | mag | PSFMAGERR_r and PSFMAGERR_i added in quadrature | |||
| imzERR | float | mag | PSFMAGERR_i and PSFMAGERR_z added in quadrature | |||
| PSFMAG_umg | float | mag | psfmag_u-psfmag_g, no extinction correction | |||
| PSFMAG_gmr | float | mag | psfmag_g-psfmag_r, no extinction correction | |||
| PSFMAG_rmi | float | mag | psfmag_r-psfmag_i, no extinction correction | |||
| PSFMAG_imz | float | mag | psfmag_i-psfmag_z, no extinction correction | |||
| PSFMAG_gmi | float | mag | psfmag_g-psfmag_i, no extinction correction | |||
| lcolor | float | mag | -0.436*uMag+1.129*gMag-0.119*rMag-0.574*iMag+0.1984 (Lenz et al.1998) | |||
| scolor | float | mag | -0.249*uMag+0.794*gMag-0.555*rMag+0.234+0.011*p1s-0.010 (Helmi et al. 2003) used in SEGUE-1 target selection, unused in SEGUE-2 | |||
| p1s | float | mag | 0.91*umg+0.415*umg-1.280 (Helmi et al. 2003) used in SEGUE-1 target selection, unused in SEGUE-2 | |||
| TOTALPM | float | mas/year | sqrt(PMRA*PMRA+PMDEC*PMDEC), in mas/year | |||
| Hg | float | mag | reduced proper motion, gMag+5*log10(TOTALPM/1000)+5 | |||
| Mi | float | mag | 4.471+7.907*imz-0.837*imz*imz used in SEGUE-1 target selection, unused in SEGUE-2 | |||
| DISTi | float | mag | 10^((iMag-Mi+5)/5.0) used in SEGUE-1 target selection, unused in SEGUE-2 | |||
| Hr | float | mag | reduced pm (uncorr r): PSFMAG_r+5*log10(TOTALPM/1000)+5 | |||
| VMI_TRANS1 | float | mag | V-I from VMAG_TRANS-(iMag-0.337*rmi-0.37) | |||
| VMI_TRANS2 | float | mag | V-I from 0.877*gmr+0.358 | |||
| VMAG_TRANS | float | mag | V mag from gMag - 0.587*gmr -0.011 | |||
| MV_TRANS | float | mag | not stuffed | |||
| DISTV_KPC | float | kpc | 10^(dmV/5.-2.) where VMAG_TRANS-(3.37*VMI_TRANS1+2.89) | |||
| VTRANS_GALREST | float | km/s | transvere velocity, km/s, derived from TOTALPM and DISTV_KPC, in a frame at rest w.r.t the Galaxy | |||
| MUTRANS_GALRADREST | float | mas/year | derived PM (mas/year) perpendicular to the Galactocentric radial vector, assuming all motion is along a Galactocentric radial vector, in a frame at rest w.r.t the Galaxy | |||
| MURAD_GALRADREST | float | mas/year | derived PM (mas/year) along the Galactocentric radial vector, assuming all motion is along a Galactocentric radial vector, in a frame at rest w.r.t the Galaxy | |||
| VTOT_GALRADREST | float | km/s | total velocioty, km/s, derived from TOTALPM and DISTV_KPC, in a frame at rest w.r.t the Galaxy | |||
| MG_TOHV | float | mag | 5.7 + 10.0*(GMR - 0.375) | |||
| VTRANS_TOHV | float | km/s | transverse velocity in Galactocentric coords, using the distance estimate from MG_TOHV which is appropriate for old stars near the MSTO and corrected for peculiar solar motion 16.6 km/s toward RA,Dec 267.5,28.1 | |||
| PM1SIGMA_TOHV | float | mas/year | Estimate of the 1-sigma error in total proper motion at this r magnitude. Formula is sqrt(4.56*4.56 + frate*2.30*2.30), where frate is 10^(0.4*(rMag-19.5)). The constants come from the Munn et al. 2004 (AJ, 127, 3034) paper describing the recalibration of USNOB with SDSS. | |||
| V1SIGMAERR_TOHV | float | km/s | The corresponding 1-sigma error in the transverse velocity based on PM1SIGMA_TOHV and the the distance estimate using MG_TOHV | |||
| TARGET_VERSION | string | version of target used |
Estimated stellar masses for BOSS galaxies using PCA technique
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| specObjID | long | Unique ID | ||||
| plate | int | Plate number | ||||
| fiberID | int | Fiber ID | ||||
| mjd | int | days | MJD of observation | |||
| ra | double | deg | Right ascension of fiber, J2000 | |||
| dec | double | deg | Declination of fiber, J2000 | |||
| z | float | Redshift used (corresponds to z_noqso in specObjAll) | ||||
| zErr | float | Error in z (corresponds to zErr_noqso in specObjAll) | ||||
| zNum | int | Index of chi^2 minimum corresponding to z_noqso | ||||
| mstellar_median | double | dex (solar masses) | median (50th percentile of PDF) of log stellar mass (best estimator) | |||
| mstellar_err | double | dex (solar masses) | 1-sigma error in log stellar mass (84th minus 16th percential) | |||
| mstellar_p2p5 | double | dex (solar masses) | 2.5th percentile of PDF of log stellar mass | |||
| mstellar_p16 | double | dex (solar masses) | 16th percentile of PDF of log stellar mass | |||
| mstellar_p84 | double | dex (solar masses) | 84th percentile of PDF of log stellar mass | |||
| mstellar_p97p5 | double | dex (solar masses) | 97.5th percentile of PDF of log stellar mass | |||
| vdisp_median | double | km/s | median (50th percentile of PDF) of velocity dispersion (best estimator) | |||
| vdisp_err | double | km/s | 1-sigma error in velocity dispersion (84th minus 16th percential) | |||
| vdisp_p2p5 | double | km/s | 2.5th percentile of PDF of velocity dispersion | |||
| vdisp_p16 | double | km/s | 16th percentile of PDF of velocity dispersion | |||
| vdisp_p84 | double | km/s | 84th percentile of PDF of velocity dispersion | |||
| vdisp_p97p5 | double | km/s | 97.5th percentile of PDF of velocity dispersion | |||
| calpha_0 | float | Coefficient for 0th eigenspectrum in fit | ||||
| calpha_1 | float | Coefficient for 1th eigenspectrum in fit | ||||
| calpha_2 | float | Coefficient for 2th eigenspectrum in fit | ||||
| calpha_3 | float | Coefficient for 3th eigenspectrum in fit | ||||
| calpha_4 | float | Coefficient for 4th eigenspectrum in fit | ||||
| calpha_5 | float | Coefficient for 5th eigenspectrum in fit | ||||
| calpha_6 | float | Coefficient for 6th eigenspectrum in fit | ||||
| calpha_norm | float | Overall normalization for best-fit | ||||
| warning | int | Output warnings: 0 if everything is fine. |
Estimated stellar masses for BOSS galaxies using photometric method, assuming passive model
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| specObjID | long | Unique ID | ||||
| plate | int | Plate number | ||||
| fiberID | int | Fiber ID | ||||
| mjd | int | days | MJD of observation | |||
| ra | double | deg | Right ascension of fiber, J2000 | |||
| dec | double | deg | Declination of fiber, J2000 | |||
| z | float | Redshift used (corresponds to z_noqso in specObjAll) | ||||
| zErr | float | Error in z (corresponds to zErr_noqso in specObjAll) | ||||
| logMass | float | dex (solar masses) | Best-fit stellar mass of galaxy | |||
| minLogMass | float | dex (solar masses) | 1-sigma minimum stellar mass (where chi-squared is within minimum + 1) | |||
| maxLogMass | float | dex (solar masses) | 1-sigma maximum stellar mass (where chi-squared is within minimum + 1) | |||
| medianPDF | float | dex (solar masses) | Median value in mass PDF (log base 10 in solar masses) | |||
| PDF16 | float | dex (solar masses) | 16% lower limit on stellar mass in PDF | |||
| PDF84 | float | dex (solar masses) | 84% upper limit on stellar mass in PDF | |||
| peakPDF | float | dex (solar masses) | Peak of PDF (log base 10 in solar masses) | |||
| logMass_noMassLoss | float | dex (solar masses) | Best-fit stellar mass of galaxy (log base 10 in solar masses) | |||
| minLogMass_noMassLoss | float | dex (solar masses) | 1-sigma minimum stellar mass (where chi-squared is within minimum + 1), not accounting for mass loss | |||
| maxLogMass_noMassLoss | float | dex (solar masses) | 1-sigma maximum stellar mass (where chi-squared is within minimum + 1), not accounting for mass loss | |||
| medianPDF_noMassLoss | float | dex (solar masses) | Median value in mass PDF, not accounting for mass loss (log base 10 in solar masses) | |||
| PDF16_noMassLoss | float | dex (solar masses) | 16% lower limit on stellar mass in PDF, not accounting for mass loss | |||
| PDF84_noMassLoss | float | dex (solar masses) | 84% upper limit on stellar mass in PDF, not accounting for mass loss | |||
| peakPDF_noMassLoss | float | dex (solar masses) | Peak of PDF, not accounting for mass loss (log base 10 in solar masses) | |||
| reducedChi2 | float | Reduced chi squared of best fit | ||||
| age | float | Gyrs | Age of best fit | |||
| minAge | float | Gyrs | 1-sigma minimum age (where chi-squared is within minimum + 1) | |||
| maxAge | float | Gyrs | 1-sigma maximum age (where chi-squared is within minimum + 1) | |||
| SFR | float | solar masses per year | Star-formation rate of best fit | |||
| minSFR | float | solar masses per year | 1-sigma minimum star-formation rate of best fit (where chi-squared is within minimum + 1) | |||
| maxSFR | float | solar masses per year | 1-sigma maximum star-formation rate of best fit (where chi-squared is within minimum + 1) | |||
| absMagK | float | Absolute magnitude in K inferred from model | ||||
| SFH | string | Star-formation history model used | ||||
| Metallicity | string | Metallicity of best fit template (0.004, 0.01, 0.02, 0.04, or "composite") | ||||
| reddeninglaw | int | ID of best fit reddening law (0 = no reddening) | ||||
| nFilter | int | Number of filters used in the fit (default is 5 for ugriz) |
Estimated stellar masses for BOSS galaxies using photometric method, assuming a star-forming model
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| specObjID | long | Unique ID | ||||
| plate | int | Plate number | ||||
| fiberID | int | Fiber ID | ||||
| mjd | int | days | MJD of observation | |||
| ra | double | deg | Right ascension of fiber, J2000 | |||
| dec | double | deg | Declination of fiber, J2000 | |||
| z | float | Redshift used (corresponds to z_noqso in specObjAll) | ||||
| zErr | float | Error in z (corresponds to zErr_noqso in specObjAll) | ||||
| logMass | float | dex (solar masses) | Best-fit stellar mass of galaxy | |||
| minLogMass | float | dex (solar masses) | 1-sigma minimum stellar mass (where chi-squared is within minimum + 1) | |||
| maxLogMass | float | dex (solar masses) | 1-sigma maximum stellar mass (where chi-squared is within minimum + 1) | |||
| medianPDF | float | dex (solar masses) | Median value in mass PDF (log base 10 in solar masses) | |||
| PDF16 | float | dex (solar masses) | 16% lower limit on stellar mass in PDF | |||
| PDF84 | float | dex (solar masses) | 84% upper limit on stellar mass in PDF | |||
| peakPDF | float | dex (solar masses) | Peak of PDF (log base 10 in solar masses) | |||
| logMass_noMassLoss | float | dex (solar masses) | Best-fit stellar mass of galaxy (log base 10 in solar masses) | |||
| minLogMass_noMassLoss | float | dex (solar masses) | 1-sigma minimum stellar mass (where chi-squared is within minimum + 1), not accounting for mass loss | |||
| maxLogMass_noMassLoss | float | dex (solar masses) | 1-sigma maximum stellar mass (where chi-squared is within minimum + 1), not accounting for mass loss | |||
| medianPDF_noMassLoss | float | dex (solar masses) | Median value in mass PDF, not accounting for mass loss (log base 10 in solar masses) | |||
| PDF16_noMassLoss | float | dex (solar masses) | 16% lower limit on stellar mass in PDF, not accounting for mass loss | |||
| PDF84_noMassLoss | float | dex (solar masses) | 84% upper limit on stellar mass in PDF, not accounting for mass loss | |||
| peakPDF_noMassLoss | float | dex (solar masses) | Peak of PDF, not accounting for mass loss (log base 10 in solar masses) | |||
| reducedChi2 | float | Reduced chi squared of best fit | ||||
| age | float | Gyrs | Age of best fit | |||
| minAge | float | Gyrs | 1-sigma minimum age (where chi-squared is within minimum + 1) | |||
| maxAge | float | Gyrs | 1-sigma maximum age (where chi-squared is within minimum + 1) | |||
| SFR | float | solar masses per year | Star-formation rate of best fit | |||
| minSFR | float | solar masses per year | 1-sigma minimum star-formation rate of best fit (where chi-squared is within minimum + 1) | |||
| maxSFR | float | solar masses per year | 1-sigma maximum star-formation rate of best fit (where chi-squared is within minimum + 1) | |||
| absMagK | float | Absolute magnitude in K inferred from model | ||||
| SFH | string | Star-formation history model used ("const" or "tau=X" or "trunc=X", where X is the exponential decline rate, or the time until truncation of the model) | ||||
| Metallicity | string | Metallicity of best fit template (0.004, 0.01, 0.02, 0.04, or "composite") | ||||
| reddeninglaw | int | ID of best fit reddening law (0 = no reddening) | ||||
| nFilter | int | Number of filters used in the fit (default is 5 for ugriz) |
Full list of all 'things': unique objects in the SDSS imagin
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| thingId | long | thing ID number | ||||
| sdssPolygonID | int | id number of polygon containing object in sdssPolygons | ||||
| fieldID | long | field identification of primary field | ||||
| objID | long | id of object for primary (or best) observation | ||||
| isPrimary | int | Non-zero if there is a detection of this object in the primary field covering this balkan. | ||||
| nDetect | int | Number of detections of this object. | ||||
| nEdge | int | Number of fields in which this is a RUN_EDGE object (observation close to edge) | ||||
| ra | double | DR8 Right ascension, J2000 deg | ||||
| dec | double | DR8 Declination, J2000 deg | ||||
| loadVersion | int | Load Version |
Measures of classification confidence from Galaxy Zoo
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| specobjid | long | match to DR8 spectrum object | ||||
| objid | long | DR8 ObjID | ||||
| dr7objid | long | DR7 ObjID | ||||
| ra | float | Right Ascension, J2000 deg | ||||
| dec | float | Declination, J2000 deg | ||||
| rastring | string | Right ascension in sexagesimal | ||||
| decstring | string | Declination in sexagesimal | ||||
| f_unclass_clean | double | fraction of galaxies in same bin that are unclassified, clean condition | ||||
| f_misclass_clean | double | fraction of galaxies in same bin that are misclassified, clean condition | ||||
| avcorr_clean | double | average bias correction in bin, clean condition | ||||
| stdcorr_clean | double | std dev of bias corrections in bin, clean condition | ||||
| f_misclass_greater | double | fraction of galaxies in same bin that are misclassified, greater condition | ||||
| avcorr_greater | double | average bias correction in bin, greater condition | ||||
| stdcorr_greater | double | std dev of bias corrections in bin, greater condition |
Results from the bias study using mirrored images from Galaxy Zo
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| specobjid | long | match to DR8 spectrum object | ||||
| objid | long | DR8 ObjID | ||||
| dr7objid | long | DR7 ObjID | ||||
| ra | float | Right Ascension, J2000 deg | ||||
| dec | float | Declination, J2000 deg | ||||
| rastring | string | Right ascension in sexagesimal | ||||
| decstring | string | Declination in sexagesimal | ||||
| nvote_mr1 | int | number of votes, vertical mirroring | ||||
| p_el_mr1 | double | fraction of votes for elliptical, vertical mirroring | ||||
| p_cw_mr1 | double | fraction of votes for clockwise spiral, vertical mirroring | ||||
| p_acw_mr1 | double | fraction of votes for anticlockwise spiral, vertical mirroring | ||||
| p_edge_mr1 | double | fraction of votes for edge-on disk, vertical mirroring | ||||
| p_dk_mr1 | double | fraction of votes for don't know, vertical mirroring | ||||
| p_mg_mr1 | double | fraction of votes for merger, vertical mirroring | ||||
| p_cs_mr1 | double | fraction of votes for combined spiral, vertical mirroring | ||||
| nvote_mr2 | int | number of votes, diagonal mirroring | ||||
| p_el_mr2 | double | fraction of votes for elliptical, diagonal mirroring | ||||
| p_cw_mr2 | double | fraction of votes for clockwise spiral, diagonal mirroring | ||||
| p_acw_mr2 | double | fraction of votes for anticlockwise spiral, diagonal mirroring | ||||
| p_edge_mr2 | double | fraction of votes for edge-on disk, diagonal mirroring | ||||
| p_dk_mr2 | double | fraction of votes for don't know, diagonal mirroring | ||||
| p_mg_mr2 | double | fraction of votes for merger, diagonal mirroring | ||||
| p_cs_mr2 | double | fraction of votes for combined spiral, diagonal mirroring |
Results from the bias study that introduced monochrome images in Galaxy Zoo
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| specobjid | long | match to DR8 spectrum object | ||||
| objid | long | DR8 ObjID | ||||
| dr7objid | long | DR7 ObjID | ||||
| ra | float | Right Ascension, J2000 deg | ||||
| dec | float | Declination, J2000 deg | ||||
| rastring | string | Right ascension in sexagesimal | ||||
| decstring | string | Declination in sexagesimal | ||||
| nvote_mon | int | number of votes, monochrome | ||||
| p_el_mon | double | fraction of votes for elliptical, monochrome | ||||
| p_cw_mon | double | fraction of votes for clockwise spiral, monochrome | ||||
| p_acw_mon | double | fraction of votes for anticlockwise spiral, monochrome | ||||
| p_edge_mon | double | fraction of votes for edge-on disk, monochrome | ||||
| p_dk_mon | double | fraction of votes for don't know, monochrome | ||||
| p_mg_mon | double | fraction of votes for merger, monochrome | ||||
| p_cs_mon | double | fraction of votes for combined spiral (cw + acw + edge-on), monochrome |
Morphology classifications of galaxies without spectra from Galaxy Zo
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| specobjid | long | match to DR8 spectrum object | ||||
| objid | long | DR8 ObjID | ||||
| dr7objid | long | DR7 ObjID | ||||
| ra | float | Right Ascension, J2000 deg | ||||
| dec | float | Declination, J2000 deg | ||||
| rastring | string | Right ascension in sexagesimal | ||||
| nvote | int | number of votes | ||||
| p_el | double | fraction of votes for elliptical | ||||
| p_cw | double | fraction of votes for clockwise spiral | ||||
| p_acw | double | fraction of votes for anticlockwise spiral | ||||
| p_edge | double | fraction of votes for edge-on disk | ||||
| p_dk | double | fraction of votes for don't know | ||||
| p_mg | double | fraction of votes for merger | ||||
| p_cs | double | fraction of votes for combined spiral - cw + acw + edge-on |
Morphological classifications of spectroscopic galaxies from Galaxy Zo
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| specobjid | long | match to DR8 spectrum object | ||||
| objid | long | DR8 ObjID | ||||
| dr7objid | long | DR7 ObjID | ||||
| ra | float | Right Ascension, J2000 deg | ||||
| dec | float | Declination, J2000 deg | ||||
| rastring | string | Right ascension in sexagesimal | ||||
| decstring | string | Declination in sexagesimal | ||||
| nvote | int | number of votes | ||||
| p_el | double | fraction of votes for elliptical | ||||
| p_cw | double | fraction of votes for clockwise spiral | ||||
| p_acw | double | fraction of votes for anticlockwise spiral | ||||
| p_edge | double | fraction of votes for edge-on disk | ||||
| p_dk | double | fraction of votes for don't know | ||||
| p_mg | double | fraction of votes for merger | ||||
| p_cs | double | fraction of votes for combined spiral - cw + acw + edge-on | ||||
| p_el_debiased | double | debiased fraction of votes for elliptical | ||||
| p_cs_debiased | double | debiased fraction of votes for combined spiral | ||||
| spiral | int | flag for combined spiral - 1 if debiased spiral fraction > 0.8, 0 otherwise | ||||
| elliptical | int | flag for elliptical - 1 if debiased elliptical fraction > 0.8, 0 otherwise | ||||
| uncertain | int | flag for uncertain type - 1 if both spiral and elliptical flags are 0 |
Vote breakdown in Galaxy Zoo results
| Column | Type | Units | UCD | Error | Description | Links |
|---|---|---|---|---|---|---|
| specobjid | long | match to DR8 spectrum object | ||||
| objid | long | DR8 ObjID | ||||
| dr7objid | long | DR7 ObjID | ||||
| ra | float | Right Ascension, J2000 deg | ||||
| dec | float | Declination, J2000 deg | ||||
| rastring | string | Right ascension in sexagesimal | ||||
| decstring | string | Declination in sexagesimal | ||||
| nvote_tot | int | Total votes | ||||
| nvote_std | int | Total votes for the standard classification | ||||
| nvote_mr1 | int | Total votes for the vertical mirrored classification | ||||
| nvote_mr2 | int | Total votes for the diagonally mirrored classification | ||||
| nvote_mon | int | Total votes for the monochrome classification | ||||
| p_el | double | Fraction of votes for elliptical | ||||
| p_cw | double | Fraction of votes for clockwise spiral | ||||
| p_acw | double | Fraction of votes for anticlockwise spiral | ||||
| p_edge | double | Fraction of votes for edge-on disk | ||||
| p_dk | double | Fraction of votes for don't know | ||||
| p_mg | double | Fraction of votes for merger | ||||
| p_cs | double | Fraction of votes for combined spiral - cw + acw + edge-on |