Fastspec Data Model
- Summary:
Spectrophotometric fitting results.
- Naming Convention:
fastspec-SURVEY-PROGRAM-HEALPIX.fits.gz, whereSURVEYis the survey name (e.g., main or sv3),PROGRAMis the program name (e.g., bright or dark), andHEALPIXis the healpixel number.- Regex:
fastspec-(cmx|main|special|sv1|sv2|sv3)-(backup|bright|dark|other)-[0-9]+\.fits.gz- File Type:
FITS
Contents
Number |
EXTNAME |
Type |
Contents |
|---|---|---|---|
PRIMARY |
IMAGE |
Keywords only. |
|
METADATA |
BINTABLE |
Table with sample metadata. |
|
SPECPHOT |
BINTABLE |
Table with spectrophotometric quantities. |
|
FASTSPEC |
BINTABLE |
Table with spectral fitting results. |
|
MODELS |
IMAGE |
Model continuum, smooth continuum, and emission-line spectra. |
FITS Header Units
HDU00
EXTNAME = PRIMARY
Required Header Keywords
Required Header Keywords Table
KEY |
Example Value |
Type |
Comment |
|---|---|---|---|
SPECPROD |
iron |
str |
Spectroscopic production name. |
COADDTYP |
healpix |
str |
Type of spectral coadd (healpix|cumulative|pernight|perexp). |
INPUTZ |
F |
bool |
Input redshifts provided. |
INPUTS |
F |
bool |
Input seeds provided. |
CONSAGE |
F |
bool |
Stellar population synthesis ages constrained by redshift. |
USEQNET |
T |
bool |
QuasarNet redshifts used where applicable. |
NMONTE |
50 |
int |
Number of Monte Carlo realizations. |
SEED |
1 |
int |
Random seed used for Monte Carlo realizations. |
NOSCORR |
F |
bool |
No smooth continuum correction derived. |
NOPHOTO |
F |
bool |
No fitting to photometry carried out. |
BRDLFIT |
T |
bool |
Broad Balmer emission-line modeling attempted. |
UFLOOR |
0.01 |
float |
Spectroscopic fractional uncertainty floor. |
SNRBBALM |
2.5 |
float |
Minimum broad Balmer signal-to-noise ratio. |
CHECKSUM |
ZHWHZHVFZHVFZHVF |
str |
HDU checksum updated 2022-08-02T19:06:22 |
DATASUM |
0 |
str |
data unit checksum updated 2022-08-02T19:06:22 |
Empty HDU.
HDU01
EXTNAME = METADATA
Metadata associated with each object fitted.
Required Header Keywords
Required Header Keywords Table
KEY |
Example Value |
Type |
Comment |
|---|---|---|---|
NAXIS1 |
339 |
int |
length of dimension 1 |
NAXIS2 |
338 |
int |
length of dimension 2 |
CHECKSUM |
hFY6jCV3hCV3hCV3 |
str |
HDU checksum updated 2022-08-03T14:25:08 |
DATASUM |
1759692941 |
str |
data unit checksum updated 2022-08-03T14:25:08 |
Required Data Table Columns
Name |
Type |
Units |
Description |
|---|---|---|---|
TARGETID |
int64 |
Unique target ID. |
|
SURVEY [1] |
bytes3 |
Survey name. |
|
PROGRAM [1] |
bytes6 |
Program name. |
|
HEALPIX [1] |
int32 |
Healpixel number. |
|
TILEID [2] |
int32 |
Tile ID number. |
|
FIBER [2] |
int32 |
Fiber number. |
|
NIGHT [2] |
int32 |
Night of observation. |
|
EXPID [3] |
int32 |
Exposure ID number. |
|
TILEID_LIST |
str? |
List of tile IDs that went into healpix coadd. |
|
RA |
float64 |
deg |
Right ascension from target catalog. |
DEC |
float64 |
deg |
Declination from target catalog. |
COADD_FIBERSTATUS |
int64 |
Fiber status bit. |
|
CMX_TARGET [5] |
int64 |
Commissioning (CMX) targeting bit. |
|
DESI_TARGET |
int64 |
DESI targeting bit. |
|
BGS_TARGET |
int64 |
BGS targeting bit. |
|
MWS_TARGET |
int64 |
MWS targeting bit. |
|
SCND_TARGET |
int64 |
Secondary target targeting bit. |
|
SV1_DESI_TARGET [5] |
int64 |
SV1 DESI targeting bit. |
|
SV1_BGS_TARGET [5] |
int64 |
SV1 BGS targeting bit. |
|
SV1_MWS_TARGET [5] |
int64 |
SV1 MWS targeting bit. |
|
SV2_DESI_TARGET [5] |
int64 |
SV2 DESI targeting bit. |
|
SV2_BGS_TARGET [5] |
int64 |
SV2 BGS targeting bit. |
|
SV2_MWS_TARGET [5] |
int64 |
SV2 MWS targeting bit. |
|
SV3_DESI_TARGET [5] |
int64 |
SV3 DESI targeting bit. |
|
SV3_BGS_TARGET [5] |
int64 |
SV3 BGS targeting bit. |
|
SV3_MWS_TARGET [5] |
int64 |
SV3 MWS targeting bit. |
|
SV1_SCND_TARGET [5] |
int64 |
SV1 secondary targeting bit. |
|
SV2_SCND_TARGET [5] |
int64 |
SV2 secondary targeting bit. |
|
SV3_SCND_TARGET [5] |
int64 |
SV3 secondary targeting bit. |
|
Z |
float64 |
Redshift based on either Redrock or QuasarNet (for QSO targets only). |
|
ZWARN |
int8 |
Redshift zwarning bit based on either Redrock or QuasarNet (for QSO targets only). |
|
DELTACHI2 |
float64 |
Redrock delta-chi-squared. |
|
SPECTYPE |
str6 |
Redrock spectral classification type. |
|
SUBTYPE |
str20 |
Redrock spectral subtype. |
|
Z_RR |
float64 |
Redrock redshift. |
|
ZWARN_RR |
int8 |
Redrock zwarning bit. |
|
TSNR2_BGS |
float32 |
Template signal-to-noise ratio squared for BGS targets. |
|
TSNR2_LRG |
float32 |
Like TSNR2_BGS but for LRG targets. |
|
TSNR2_ELG |
float32 |
Like TSNR2_BGS but for ELG targets. |
|
TSNR2_QSO |
float32 |
Like TSNR2_BGS but for QSO targets. |
|
TSNR2_LYA |
float32 |
Like TSNR2_BGS but for LYA targets. |
|
PHOTSYS |
str1 |
Photometric system (N or S). |
|
LS_ID |
int64 |
Unique Legacy Surveys identification number. |
|
FIBERFLUX_G |
float32 |
nmgy |
Fiber g-band flux corrected for Galactic extinction. |
FIBERFLUX_R |
float32 |
nmgy |
Like FIBERFLUX_G but for the r-band. |
FIBERFLUX_Z |
float32 |
nmgy |
Like FIBERFLUX_G but for the z-band. |
FIBERTOTFLUX_G |
float32 |
nmgy |
Fibertot g-band flux corrected for Galactic extinction. |
FIBERTOTFLUX_R |
float32 |
nmgy |
Like FIBERTOTFLUX_G but for the r-band. |
FIBERTOTFLUX_Z |
float32 |
nmgy |
Like FIBERTOTFLUX_G but for the z-band. |
FLUX_G |
float32 |
nmgy |
Total g-band flux corrected for Galactic extinction. |
FLUX_R |
float32 |
nmgy |
Like FLUX_G but for the r-band. |
FLUX_Z |
float32 |
nmgy |
Like FLUX_G but for the z-band. |
FLUX_W1 |
float32 |
nmgy |
Like FLUX_G but for the W1-band. |
FLUX_W2 |
float32 |
nmgy |
Like FLUX_G but for the W2-band. |
FLUX_W3 |
float32 |
nmgy |
Like FLUX_G but for the W3-band. |
FLUX_W4 |
float32 |
nmgy |
Like FLUX_G but for the W4-band. |
FLUX_IVAR_G |
float32 |
1 / nmgy2 |
Inverse variance of FLUX_G corrected for Galactic extinction. |
FLUX_IVAR_R |
float32 |
1 / nmgy2 |
Like FLUX_IVAR_G but for the r-band. |
FLUX_IVAR_Z |
float32 |
1 / nmgy2 |
Like FLUX_IVAR_G but for the z-band. |
FLUX_IVAR_W1 |
float32 |
1 / nmgy2 |
Like FLUX_IVAR_G but for the W1-band. |
FLUX_IVAR_W2 |
float32 |
1 / nmgy2 |
Like FLUX_IVAR_G but for the W2-band. |
FLUX_IVAR_W3 |
float32 |
1 / nmgy2 |
Like FLUX_IVAR_G but for the W3-band. |
FLUX_IVAR_W4 |
float32 |
1 / nmgy2 |
Like FLUX_IVAR_G but for the W4-band. |
EBV |
float32 |
mag |
Milky Way foreground color excess. |
MW_TRANSMISSION_G |
float32 |
Milky Way foreground dust transmission factor [0-1] in the g-band. |
|
MW_TRANSMISSION_R |
float32 |
Like MW_TRANSMISSION_G but for the r-band. |
|
MW_TRANSMISSION_Z |
float32 |
Like MW_TRANSMISSION_G but for the z-band. |
|
MW_TRANSMISSION_W1 |
float32 |
Like MW_TRANSMISSION_G but for the W1-band. |
|
MW_TRANSMISSION_W2 |
float32 |
Like MW_TRANSMISSION_G but for the W2-band. |
|
MW_TRANSMISSION_W3 |
float32 |
Like MW_TRANSMISSION_G but for the W3-band. |
|
MW_TRANSMISSION_W4 |
float32 |
Like MW_TRANSMISSION_G but for the W4-band. |
HDU02
EXTNAME = SPECPHOT
Table with spectrophotometric quantities.
Required Header Keywords
Required Header Keywords Table
KEY |
Example Value |
Type |
Comment |
|---|---|---|---|
NAXIS1 |
3115 |
int |
length of dimension 1 |
NAXIS2 |
338 |
int |
length of dimension 2 |
CHECKSUM |
WLDnaKDlWKDlaKDl |
str |
HDU checksum updated 2022-08-03T14:25:08 |
DATASUM |
756558178 |
str |
data unit checksum updated 2022-08-03T14:25:08 |
Required Data Table Columns
Name |
Type |
Units |
Description |
|---|---|---|---|
TARGETID |
int64 |
Unique target ID. |
|
SURVEY [1] |
bytes3 |
Survey name. |
|
PROGRAM [1] |
bytes6 |
Program name. |
|
HEALPIX [1] |
int32 |
Healpixel number. |
|
TILEID [2] |
int32 |
Tile ID number. |
|
NIGHT [2] |
int32 |
Night of observation. |
|
FIBER [2] |
int32 |
Fiber number. |
|
EXPID [3] |
int32 |
Exposure ID number. |
|
SEED |
int64 |
Random seed used for Monte Carlo realizations. |
|
COEFF |
float32[5] |
1e-17 erg / (Angstrom cm2 s) |
Stellar continuum coefficients. |
RCHI2 |
float32 |
Reduced chi-squared of the full-spectrophotometric fit. |
|
RCHI2_LINE |
float32 |
Reduced chi-squared of the emission-line model fit. |
|
RCHI2_CONT |
float32 |
Reduced chi-squared of the fit to the stellar continuum. |
|
RCHI2_PHOT |
float32 |
Reduced chi-squared of the fit to the broadband photometry. |
|
VDISP |
float32 |
km / s |
Stellar velocity dispersion. |
VDISP_IVAR |
float32 |
s2 / km2 |
Inverse variance of VDISP. |
TAUV |
float32 |
V-band dust optical depth of the integrated stellar population. |
|
TAUV_IVAR |
float32 |
Inverse variance of TAUV. |
|
AGE |
float32 |
Gyr |
Light-weighted age. |
AGE_IVAR |
float32 |
1 / Gyr2 |
Inverse variance of AGE. |
ZZSUN |
float32 |
Logarithmic stellar metallicity relative to solar. |
|
ZZSUN_IVAR |
float32 |
Inverse variance of ZZSUN. |
|
LOGMSTAR |
float32 |
Msun |
Logarithmic stellar mass (h=1.0, Chabrier+2003 initial mass function). |
LOGMSTAR_IVAR |
float32 |
1 / Msun2 |
Inverse variance of LOGMSTAR. |
SFR |
float32 |
Msun / yr |
Instantaneous star formation rate (h=1.0, Chabrier+2003 initial mass function). |
SFR_IVAR |
float32 |
yr2 / Msun2 |
Inverse variance of SFR. |
DN4000 |
float32 |
Narrow 4000-A break index (from Balogh et al. 1999) measured from the emission-line subtracted spectrum. |
|
DN4000_OBS |
float32 |
Narrow 4000-A break index measured from the observed spectrum. |
|
DN4000_IVAR |
float32 |
Inverse variance of DN4000_OBS and of DN4000. |
|
DN4000_MODEL |
float32 |
Narrow 4000-A break index measured from the best-fitting continuum model. |
|
DN4000_MODEL_IVAR |
float32 |
Inverse variance of DN4000_MODEL. |
|
FLUX_SYNTH_G |
float32 |
nmgy |
g-band flux (in the PHOTSYS photometric system) synthesized from the observed spectrum. |
FLUX_SYNTH_R |
float32 |
nmgy |
Like FLUX_SYNTH_G but for the r-band. |
FLUX_SYNTH_Z |
float32 |
nmgy |
Like FLUX_SYNTH_G but for the z-band. |
FLUX_SYNTH_SPECMODEL_G |
float32 |
nmgy |
g-band flux (in the PHOTSYS photometric system) synthesized from the best-fitting spectroscopic model. |
FLUX_SYNTH_SPECMODEL_R |
float32 |
nmgy |
Like FLUX_SYNTH_SPECMODEL_G but in the r-band. |
FLUX_SYNTH_SPECMODEL_Z |
float32 |
nmgy |
Like FLUX_SYNTH_SPECMODEL_G but in the z-band. |
FLUX_SYNTH_PHOTMODEL_G |
float32 |
nmgy |
g-band flux (in the PHOTSYS photometric system) synthesized from the best-fitting photometric continuum model. |
FLUX_SYNTH_PHOTMODEL_R |
float32 |
nmgy |
Like FLUX_SYNTH_PHOTMODEL_G but in the r-band. |
FLUX_SYNTH_PHOTMODEL_Z |
float32 |
nmgy |
Like FLUX_SYNTH_PHOTMODEL_G but in the z-band. |
FLUX_SYNTH_PHOTMODEL_W1 |
float32 |
nmgy |
Like FLUX_SYNTH_PHOTMODEL_G but in the W1-band. |
FLUX_SYNTH_PHOTMODEL_W2 |
float32 |
nmgy |
Like FLUX_SYNTH_PHOTMODEL_G but in the W2-band. |
FLUX_SYNTH_PHOTMODEL_W3 |
float32 |
nmgy |
Like FLUX_SYNTH_PHOTMODEL_G but in the W3-band. |
FLUX_SYNTH_PHOTMODEL_W4 |
float32 |
nmgy |
Like FLUX_SYNTH_PHOTMODEL_G but in the W4-band. |
ABSMAG10_DECAM_G [4] |
float32 |
mag |
Absolute magnitude in DECam g-band band-shifted to z=1.0 assuming h=1.0. |
ABSMAG10_IVAR_DECAM_G |
float32 |
1 / mag2 |
Inverse variance corresponding to ABSMAG10_DECAM_G. |
ABSMAG10_SYNTH_DECAM_G |
float32 |
mag |
Synthesized absolute magnitude in DECam g-band band-shifted to z=1.0 assuming h=1.0. |
ABSMAG10_SYNTH_IVAR_DECAM_G |
float32 |
1 / mag2 |
Inverse variance corresponding to ABSMAG10_SYNTH_DECAM_G. |
ABSMAG10_DECAM_R [4] |
float32 |
mag |
Like ABSMAG10_DECAM_G but for DECam r-band. |
ABSMAG10_IVAR_DECAM_R |
float32 |
1 / mag2 |
Like ABSMAG10_IVAR_DECAM_G but for DECam r-band. |
ABSMAG10_SYNTH_DECAM_R |
float32 |
mag |
Like ABSMAG10_SYNTH_DECAM_G but for DECam r-band. |
ABSMAG10_SYNTH_IVAR_DECAM_R |
float32 |
1 / mag2 |
Like ABSMAG10_SYNTH_IVAR_DECAM_G but for DECam r-band. |
ABSMAG10_DECAM_Z [4] |
float32 |
mag |
Like ABSMAG10_DECAM_G but for DECam z-band. |
ABSMAG10_IVAR_DECAM_Z |
float32 |
1 / mag2 |
Like ABSMAG10_IVAR_DECAM_G but for DECam z-band. |
ABSMAG10_SYNTH_DECAM_Z |
float32 |
mag |
Like ABSMAG10_SYNTH_DECAM_G but for DECam z-band. |
ABSMAG10_SYNTH_IVAR_DECAM_Z |
float32 |
1 / mag2 |
Like ABSMAG10_SYNTH_IVAR_DECAM_G but for DECam z-band. |
ABSMAG00_U [4] |
float32 |
mag |
Absolute magnitude in Johnson/Cousins U-band band-shifted to z=0.0 assuming h=1.0. |
ABSMAG00_IVAR_U |
float32 |
1 / mag2 |
Inverse variance corresponding to ABSMAG00_U. |
ABSMAG00_SYNTH_U |
float32 |
mag |
Synthesized absolute magnitude in Johnson/Cousins U-band band-shifted to z=0.0 assuming h=1.0. |
ABSMAG00_SYNTH_IVAR_U |
float32 |
1 / mag2 |
Inverse variance corresponding to ABSMAG00_SYNTH_U. |
ABSMAG00_B [4] |
float32 |
mag |
Like ABSMAG00_U but for Johnson/Cousins B-band. |
ABSMAG00_IVAR_B |
float32 |
1 / mag2 |
Like ABSMAG00_IVAR_U but for Johnson/Cousins B-band. |
ABSMAG00_SYNTH_B |
float32 |
mag |
Like ABSMAG00_SYNTH_U but for Johnson/Cousins B-band. |
ABSMAG00_SYNTH_IVAR_B |
float32 |
1 / mag2 |
Like ABSMAG00_SYNTH_IVAR_U but for Johnson/Cousins B-band. |
ABSMAG00_V [4] |
float32 |
mag |
Like ABSMAG00_U but for Johnson/Cousins V-band. |
ABSMAG00_IVAR_V |
float32 |
1 / mag2 |
Like ABSMAG00_IVAR_U but for Johnson/Cousins V-band. |
ABSMAG00_SYNTH_V |
float32 |
mag |
Like ABSMAG00_SYNTH_U but for Johnson/Cousins V-band. |
ABSMAG00_SYNTH_IVAR_V |
float32 |
1 / mag2 |
Like ABSMAG00_SYNTH_IVAR_U but for Johnson/Cousins V-band. |
ABSMAG00_TWOMASS_J [4] |
float32 |
mag |
Absolute magnitude in 2MASS J-band band-shifted to z=0.0 assuming h=1.0. |
ABSMAG00_IVAR_TWOMASS_J |
float32 |
1 / mag2 |
Inverse variance corresponding to ABSMAG00_TWOMASS_J. |
ABSMAG00_SYNTH_TWOMASS_J |
float32 |
mag |
Synthesized absolute magnitude in 2MASS J-band band-shifted to z=0.0 assuming h=1.0. |
ABSMAG00_SYNTH_IVAR_TWOMASS_J |
float32 |
1 / mag2 |
Inverse variance corresponding to ABSMAG01_SYNTH_TWOMASS_J. |
ABSMAG01_SDSS_U [4] |
float32 |
mag |
Absolute magnitude in SDSS u-band band-shifted to z=0.1 assuming h=1.0. |
ABSMAG01_IVAR_SDSS_U |
float32 |
1 / mag2 |
Inverse variance corresponding to ABSMAG01_SDSS_U. |
ABSMAG01_SYNTH_SDSS_U |
float32 |
mag |
Synthesized absolute magnitude in SDSS u-band band-shifted to z=0.1 assuming h=1.0. |
ABSMAG01_SYNTH_IVAR_SDSS_U |
float32 |
1 / mag2 |
Inverse variance corresponding to ABSMAG01_SYNTH_SDSS_U. |
ABSMAG01_SDSS_G [4] |
float32 |
mag |
Like ABSMAG01_SDSS_U but for SDSS g-band. |
ABSMAG01_IVAR_SDSS_G |
float32 |
1 / mag2 |
Like ABSMAG01_IVAR_SDSS_U but for SDSS g-band. |
ABSMAG01_SYNTH_SDSS_G |
float32 |
mag |
Like ABSMAG01_SYNTH_SDSS_U but for SDSS g-band. |
ABSMAG01_SYNTH_IVAR_SDSS_G |
float32 |
1 / mag2 |
Like ABSMAG01_SYNTH_IVAR_SDSS_U but for SDSS g-band. |
ABSMAG01_SDSS_R [4] |
float32 |
mag |
Like ABSMAG01_SDSS_U but for SDSS r-band. |
ABSMAG01_IVAR_SDSS_R |
float32 |
1 / mag2 |
Like ABSMAG01_IVAR_SDSS_U but for SDSS r-band. |
ABSMAG01_SYNTH_SDSS_R |
float32 |
mag |
Like ABSMAG01_SYNTH_SDSS_U but for SDSS r-band. |
ABSMAG01_SYNTH_IVAR_SDSS_R |
float32 |
1 / mag2 |
Like ABSMAG01_SYNTH_IVAR_SDSS_U but for SDSS r-band. |
ABSMAG01_SDSS_I [4] |
float32 |
mag |
Like ABSMAG01_SDSS_U but for SDSS i-band. |
ABSMAG01_IVAR_SDSS_I |
float32 |
1 / mag2 |
Like ABSMAG01_IVAR_SDSS_U but for SDSS i-band. |
ABSMAG01_SYNTH_SDSS_I |
float32 |
mag |
Like ABSMAG01_SYNTH_SDSS_U but for SDSS i-band. |
ABSMAG01_SYNTH_IVAR_SDSS_I |
float32 |
1 / mag2 |
Like ABSMAG01_SYNTH_IVAR_SDSS_U but for SDSS i-band. |
ABSMAG01_SDSS_Z [4] |
float32 |
mag |
Like ABSMAG01_SDSS_U but for SDSS z-band. |
ABSMAG01_IVAR_SDSS_Z |
float32 |
1 / mag2 |
Like ABSMAG01_IVAR_SDSS_U but for SDSS z-band. |
ABSMAG01_SYNTH_SDSS_Z |
float32 |
mag |
Like ABSMAG01_SYNTH_SDSS_U but for SDSS z-band. |
ABSMAG01_SYNTH_IVAR_SDSS_Z |
float32 |
1 / mag2 |
Like ABSMAG01_SYNTH_IVAR_SDSS_U but for SDSS z-band. |
ABSMAG01_W1 [4] |
float32 |
mag |
Absolute magnitude in WISE W1-band band-shifted to z=0.1 assuming h=1.0. |
ABSMAG01_IVAR_W1 |
float32 |
1 / mag2 |
Inverse variance corresponding to ABSMAG01_W1. |
ABSMAG01_SYNTH_W1 |
float32 |
mag |
Synthesized absolute magnitude in WISE W1-band band-shifted to z=0.1 assuming h=1.0. |
ABSMAG01_SYNTH_IVAR_W1 |
float32 |
1 / mag2 |
Inverse variance corresponding to ABSMAG01_SYNTH_W1. |
KCORR10_DECAM_G |
float32 |
mag |
K-correction used to derive ABSMAG10_DECAM_G band-shifted to z=1.0. |
KCORR10_DECAM_R |
float32 |
mag |
Like KCORR10_DECAM_G but for DECam r-band. |
KCORR10_DECAM_Z |
float32 |
mag |
Like KCORR10_DECAM_G but for DECam z-band. |
KCORR00_U |
float32 |
mag |
K-correction used to derive ABSMAG00_U band-shifted to z=0.0. |
KCORR00_B |
float32 |
mag |
Like KCORR00_U but for Johnson/Cousins B-band. |
KCORR00_V |
float32 |
mag |
Like KCORR00_U but for Johnson/Cousins V-band. |
KCORR01_SDSS_U |
float32 |
mag |
K-correction used to derive ABSMAG01_SDSS_U band-shifted to z=0.1. |
KCORR01_SDSS_G |
float32 |
mag |
Like KCORR01_SDSS_U but for SDSS g-band. |
KCORR01_SDSS_R |
float32 |
mag |
Like KCORR01_SDSS_U but for SDSS r-band. |
KCORR01_SDSS_I |
float32 |
mag |
Like KCORR01_SDSS_U but for SDSS i-band. |
KCORR01_SDSS_Z |
float32 |
mag |
Like KCORR01_SDSS_U but for SDSS z-band. |
KCORR01_W1 |
float32 |
mag |
K-correction used to derive ABSMAG01_W1 band-shifted to z=0.0. |
LOGLNU_1500 |
float32 |
1e-28 erg / (Hz s) |
Monochromatic luminosity at 1500 A in the rest-frame. |
LOGLNU_1500_IVAR |
float32 |
1e+56 Hz2 s2 / erg2 |
Inverse variance in LOGLNU_1500. |
LOGLNU_2800 |
float32 |
1e-28 erg / (Hz s) |
Monochromatic luminosity at 2800 A in the rest-frame. |
LOGLNU_2800_IVAR |
float32 |
1e+56 Hz2 s2 / erg2 |
Inverse variance in LOGLNU_2800. |
LOGL_1450 |
float32 |
1e10 Lsun |
Integrated luminosity at 1450 A in the rest-frame. |
LOGL_1450_IVAR |
float32 |
1e-20 / Lsun2 |
Inverse variance in LOGL_1450. |
LOGL_1700 |
float32 |
1e10 Lsun |
Integrated luminosity at 1700 A in the rest-frame. |
LOGL_1700_IVAR |
float32 |
1e-20 / Lsun2 |
Inverse variance in LOGL_1700. |
LOGL_3000 |
float32 |
1e10 Lsun |
Integrated luminosity at 3000 A in the rest-frame. |
LOGL_3000_IVAR |
float32 |
1e-20 / Lsun2 |
Inverse variance in LOGL_3000. |
LOGL_5100 |
float32 |
1e10 Lsun |
Integrated luminosity at 5100 A in the rest-frame. |
LOGL_5100_IVAR |
float32 |
1e-20 / Lsun2 |
Inverse variance in LOGL_5100. |
FLYA_1215_CONT |
float32 |
1e-17 erg / (Angstrom cm2 s) |
Continuum flux at 1215.67 A in the rest-frame. |
FLYA_1215_CONT_IVAR |
float32 |
1e+34 cm4 Angstrom2 s2 / erg2 |
Inverse variance in FLYA_1215_CONT. |
FOII_3727_CONT |
float32 |
1e-17 erg / (Angstrom cm2 s) |
Continuum flux at 3728.483 A in the rest-frame. |
FOII_3727_CONT_IVAR |
float32 |
1e+34 cm4 Angstrom2 s2 / erg2 |
Inverse variance in FOII_3727_CONT. |
FHBETA_CONT |
float32 |
1e-17 erg / (Angstrom cm2 s) |
Continuum flux at 4862.683 A in the rest-frame. |
FHBETA_CONT_IVAR |
float32 |
1e+34 cm4 Angstrom2 s2 / erg2 |
Inverse variance in FHBETA_CONT. |
FOIII_5007_CONT |
float32 |
1e-17 erg / (Angstrom cm2 s) |
Continuum flux at 5008.239 A in the rest-frame. |
FOIII_5007_CONT_IVAR |
float32 |
1e+34 cm4 Angstrom2 s2 / erg2 |
Inverse variance in FOIII_5007_CONT. |
FHALPHA_CONT |
float32 |
1e-17 erg / (Angstrom cm2 s) |
Continuum flux at 6564.613 A in the rest-frame. |
FHALPHA_CONT_IVAR |
float32 |
1e+34 cm4 Angstrom2 s2 / erg2 |
Inverse variance in FHALPHA_CONT. |
HDU03
EXTNAME = FASTSPEC
Table with spectral fitting results.
Required Header Keywords
Required Header Keywords Table
KEY |
Example Value |
Type |
Comment |
|---|---|---|---|
NAXIS1 |
3115 |
int |
length of dimension 1 |
NAXIS2 |
338 |
int |
length of dimension 2 |
CHECKSUM |
WLDnaKDlWKDlaKDl |
str |
HDU checksum updated 2022-08-03T14:25:08 |
DATASUM |
756558178 |
str |
data unit checksum updated 2022-08-03T14:25:08 |
Required Data Table Columns
Name |
Type |
Units |
Description |
|---|---|---|---|
TARGETID |
int64 |
Unique target ID. |
|
SURVEY [1] |
bytes3 |
Survey name. |
|
PROGRAM [1] |
bytes6 |
Program name. |
|
HEALPIX [1] |
int32 |
Healpixel number. |
|
TILEID [2] |
int32 |
Tile ID number. |
|
NIGHT [2] |
int32 |
Night of observation. |
|
FIBER [2] |
int32 |
Fiber number. |
|
EXPID [3] |
int32 |
Exposure ID number. |
|
SNR_B |
float32 |
Median signal-to-noise ratio per pixel in the b camera. |
|
SNR_R |
float32 |
Like SNR_B but in the r camera. |
|
SNR_Z |
float32 |
Like SNR_B but in z camera. |
|
SMOOTHCORR_B |
float32 |
percent |
Median value of the smooth continuum correction relative to the data in the b camera. |
SMOOTHCORR_R |
float32 |
percent |
Like SMOOTHCORR_B but in the r camera. |
SMOOTHCORR_Z |
float32 |
percent |
Like SMOOTHCORR_B but in the z camera. |
APERCORR |
float32 |
Median aperture correction factor. |
|
APERCORR_G |
float32 |
Aperture correction factor measured in the g-band. |
|
APERCORR_R |
float32 |
Like APERCORR_G but measured in the r-band. |
|
APERCORR_Z |
float32 |
Like APERCORR_G but measured in the z-band. |
|
INIT_SIGMA_UV |
float32 |
km / s |
Initial line width for the rest-frame UV emission lines. |
INIT_SIGMA_NARROW |
float32 |
km / s |
Like INIT_SIGMA_UV but for the forbidden plus narrow Balmer emission lines. |
INIT_SIGMA_BALMER |
float32 |
km / s |
Like INIT_SIGMA_UV but for broad Balmer emission lines. |
INIT_VSHIFT_UV |
float32 |
km / s |
Initial velocity shift for the UV emission lines. |
INIT_VSHIFT_NARROW |
float32 |
km / s |
Like INIT_VSHIFT_UV but for narrow (forbidden and narrow Balmer) emission lines. |
INIT_VSHIFT_BALMER |
float32 |
km / s |
Like INIT_VSHIFT_UV but for broad Balmer emission lines. |
INIT_BALMER_BROAD |
bool |
Boolean flag indicating whether a broad Balmer emission line was initially identified in the spectral range. |
|
DELTA_LINECHI2 |
float32 |
Chi-squared difference between an emission-line model without and with broad lines. |
|
DELTA_LINENDOF |
int32 |
Difference in the degrees of freedom between an emission-line model without and with broad lines. |
|
DELTA_KINECHI2 |
float32 |
Chi-squared difference between the constrained and relaxed emission-line model. |
|
DELTA_KINENDOF |
int32 |
Difference in the degrees of freedom between the constrained and relaxed emission-line model. |
|
MGII_DOUBLET_RATIO |
float32 |
MgII 2796 / 2803 doublet line-ratio. |
|
MGII_DOUBLET_RATIO_IVAR |
float32 |
Inverse variance in MGII_DOUBLET_RATIO. |
|
OII_DOUBLET_RATIO |
float32 |
[OII] 3726 / 3729 doublet line-ratio. |
|
OII_DOUBLET_RATIO_IVAR |
float32 |
Inverse variance in OII_DOUBLET_RATIO. |
|
OIII_DOUBLET_RATIO |
float32 |
[OIII] 5007 / 4959 doublet line-ratio. |
|
OIII_DOUBLET_RATIO_IVAR |
float32 |
Inverse variance in OIII_DOUBLET_RATIO. |
|
SII_DOUBLET_RATIO |
float32 |
[SII] 6731 / 6716 doublet line-ratio. |
|
SII_DOUBLET_RATIO_IVAR |
float32 |
Inverse variance in SII_DOUBLET_RATIO. |
|
NII_DOUBLET_RATIO |
float32 |
[NII] 6584 / 6548 doublet line-ratio. |
|
NII_DOUBLET_RATIO_IVAR |
float32 |
Inverse variance in NII_DOUBLET_RATIO. |
|
OIIRED_DOUBLET_RATIO |
float32 |
[OII] 7320 / 7330 doublet (actually a quadruplet) line-ratio. |
|
OIIRED_DOUBLET_RATIO_IVAR |
float32 |
Inverse variance in OIIRED_DOUBLET_RATIO. |
|
LINENAME_MODELAMP [6] |
float32 |
1e-17 erg / (Angstrom cm2 s) |
Model emission-line amplitude (before convolution with the resolution matrix). |
LINENAME_AMP [6] |
float32 |
1e-17 erg / (Angstrom cm2 s) |
Emission line amplitude. |
LINENAME_AMP_IVAR [6] |
float32 |
1e+34 Angstrom2 cm4 s2 / erg2 |
Inverse variance in LINENAME_AMP. |
LINENAME_FLUX [6] |
float32 |
1e-17 erg / (cm2 s) |
Gaussian-integrated emission-line flux. |
LINENAME_FLUX_IVAR [6] |
float32 |
1e+34 cm4 s2 / erg2 |
Inverse variance in LINENAME_FLUX. |
LINENAME_BOXFLUX [6] |
float32 |
1e-17 erg / (cm2 s) |
Boxcar-integrated emission-line flux. |
LINENAME_BOXFLUX_IVAR [6] |
float32 |
1e+34 cm4 s2 / erg2 |
Inverse variance in LINENAME_BOXFLUX. |
LINENAME_VSHIFT [6] |
float32 |
km / s |
Velocity shift relative to Z. |
LINENAME_VSHIFT_IVAR [6] |
float32 |
s2 / km2 |
Inverse variance in LINENAME_VSHIFT. |
LINENAME_SIGMA [6] |
float32 |
km / s |
Gaussian emission-line width (before convolution with the resolution matrix). |
LINENAME_SIGMA_IVAR [6] |
float32 |
s2 / km2 |
Inverse variance in LINENAME_SIGMA. |
LINENAME_CONT [6] |
float32 |
1e-17 erg / (Angstrom cm2 s) |
Continuum flux at line center. |
LINENAME_CONT_IVAR [6] |
float32 |
1e+34 Angstrom2 cm4 s2 / erg2 |
Inverse variance in LINENAME_CONT. |
LINENAME_EW [6] |
float32 |
Angstrom |
Rest-frame emission-line equivalent width. |
LINENAME_EW_IVAR [6] |
float32 |
1 / Angstrom2 |
Inverse variance in LINENAME_EW. |
LINENAME_FLUX_LIMIT [6] |
float32 |
erg / (cm2 s) |
One-sigma upper-limit on the emission line flux. |
LINENAME_CHI2 [6] |
float32 |
Chi-squared of the line-fit. |
|
LINENAME_NPIX [6] |
int32 |
Number of pixels attributed to the emission line. |
|
LINENAME2_MOMENT1 [7] |
float32 |
Angstrom |
First moment of the continuum-subtracted pixel values within +/- 5-sigma of the Gaussian line-center. |
LINENAME2_MOMENT1_IVAR [7] |
float32 |
1 / Angstrom2 |
Inverse variance in LINENAME2_MOMENT1. |
LINENAME2_MOMENT2 [7] |
float32 |
Angstrom2 |
Second moment of the flux relative to LINENAME2_MOMENT1. |
LINENAME2_MOMENT2_IVAR [7] |
float32 |
1 / Angstrom4 |
Inverse variance in LINENAME2_MOMENT2. |
LINENAME2_MOMENT3 [7] |
float32 |
Angstrom3 |
Third moment of the flux relative to LINENAME2_MOMENT1. |
LINENAME2_MOMENT3_IVAR [7] |
float32 |
1 / Angstrom6 |
Inverse variance in LINENAME2_MOMENT3. |
HDU04
EXTNAME = MODELS
Best-fitting model spectra (corrected for Galactic extinction).
Required Header Keywords
Required Header Keywords Table
KEY |
Example Value Type Comment |
||
|---|---|---|---|
NAXIS1 |
7781 |
int |
number of pixels |
NAXIS2 |
3 |
int |
number of models |
NAXIS3 |
338 |
int |
number of objects |
BUNIT |
10**-17 erg/(s cm2 Angstrom) |
str |
flux unit |
CUNIT1 |
Angstrom |
str |
wavelength unit |
CTYPE1 |
WAVE |
str |
type of axis |
CRVAL1 |
3600.0 |
float |
wavelength of pixel CRPIX1 (Angstrom) |
CRPIX1 |
0 |
int |
0-indexed pixel number corresponding to CRVAL1 |
CDELT1 |
0.8 |
float |
pixel size (Angstrom) |
DC-FLAG |
0 |
int |
0 = linear wavelength vector |
AIRORVAC |
vac |
str |
wavelengths in vacuum (vac) |
CHECKSUM |
Q9eTT8bTQ8bTQ8bT |
str |
HDU checksum updated 2022-08-03T14:25:08 |
DATASUM |
3074907107 |
str |
data unit checksum updated 2022-08-03T14:25:08 |
Data: FITS image [int32, 7781x3,338]