SPARCL - SPARCL Field Catalog (SFC)

SPARCL Field Catalog

List of Fields available via Retrieve

CORE fields (common to all Data Sets)

Name Storage Units Description Default All
wavemin CORE AA Minimum value of wavelength coverage in Angstroms
wavemax CORE AA Maximum value of wavelength coverage in Angstroms
updated CORE Date and time when the record was created/updated
telescope CORE [Categorical] Telescope used for the observation
targetid CORE Dataset-specific photometric target identifier
spectype CORE [Categorical] Spectral type of the object (STAR, GALAXY, QSO)
specprimary CORE Whether an entry is the primary spectrum for a given target object
specid CORE Dataset-specific spectrum identifier (may not be unique)
sparcl_id CORE Universally Unique Identifier for spectrum in SPARCL
site CORE [Categorical] Site of observations
redshift_warning CORE Bitmask with warning on redshift result
redshift_err CORE Uncertainty on the measured redshift, or radial velocity in units of redshift
redshift CORE Measured redshift, or radial velocity in units of redshift
ra CORE deg Right Ascension in degrees
instrument CORE [Categorical] Instrument used for observation
file CORE File used for this record
extra_files CORE Additional files read for ingest
exptime CORE second Exposure time in seconds
dec CORE deg Declination in degrees
dateobs_center CORE Central value of the dateobs range
dateobs CORE Range of observational dates for a given spectrum (single value for a single date)
datasetgroup CORE [Categorical] Common name for a coherent set of spectra published as a single release (e.g., SDSS_BOSS)
data_release CORE [Categorical] Data release of a given record (with a common data structure, e.g., SDSS-DR16, BOSS-DR16)
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AUX and SPECTRA fields (unique to each Data Set)

Data Set: BOSS-DR16, AUX fields

Name Storage Units Description Default All
targetobjid AUX Unique database ID of targeting object based on RUN, RERUN, CAMCOl, FIELD, ID (same as SkyServer version)
class_person AUX Visual-inspection classification (0=not inspected or unknown, 1=star, 2=narrow emission-line galaxy, 3=QSO, 4=galaxy)
platerun AUX Drilling run that this plate was drilled in
fracnsiglo AUX Fraction of pixels low by more than N sigma relative to best-fit (for 1,2,..,10 sigma)
spectrographid AUX Which spectrograph (1 or 2)
eboss_target0 AUX SEQUELS, TDSS and SPIDERS target selection flags
elodie_teff AUX Kelvin Effective temperature of ELODIE star
chi68p AUX 68-th percentile value of abs(chi) of the best-fit synthetic spectrum to the actual spectrum (around 1.0 for a good fit)
plate AUX Plate number (each plate corresponds to an actual plug plate)
vdispnpix AUX Number of pixels overlapping the templates used in the velocity dispersion fit
chunk AUX Name of tiling chunk that this spectrum was tiled in (boss1, boss2, etc), important for tracking large-scale structure samples
sectarget AUX Deprecated version of secondary (calibration) target flags (meanings highly overloaded)
speclegacy AUX Set to 1 for primary SDSS Legacy program observation of object, 0 otherwise
firstrelease AUX Name of first release this PLATE, MJD, FIBERID, RUN2D was associated with
eboss_target2 AUX eBOSS, TDSS and SPIDERS target selection flags for main eBOSS survey
rchi2 AUX Reduced chi-squared of best fit
vdispdof AUX Number of degrees of freedom in velocity dispersion fit
deredsn2 AUX Dereddened overall signal-to-noise-squared measure for plate (only for BOSS spectrograph plates)
segue1_target1 AUX Primary (science) target flags for SEGUE-1 targets
mjd AUX days Modified Julian Day of observation
platequality AUX Final quality of plate this spectrum came from (good, marginal, or bad)
class_noqso AUX Spectroscopic classification for Z_NOQSO redshift
calibflux_ivar AUX nanomaggy-2 Inverse variances of ugriz fluxes used for calibrations
spectroflux_ivar AUX nanomaggy-2 Inverse variance of spectrum projected onto ugriz filters
fracnsighi AUX Fraction of pixels high by more than N sigma relative to best-fit (for 1,2,..,10 sigma)

Data Set: BOSS-DR16, SPECTRA fields

Name Storage Units Description Default All
wave_sigma SPECTRA pixel Line-spread function width (sigma of approximating Gaussian) in units of number of pixel
wavelength SPECTRA AA Wavelength in units of Angstroms
sky SPECTRA 1e-17 erg cm-2 s-1 AA-1 Subtracted sky flux
model SPECTRA 1e-17 erg cm-2 s-1 AA-1 Pipeline best model fit used for classification and redshift
mask SPECTRA and_mask
ivar SPECTRA 1e+34 cm4 s2 AA2 erg-2 Inverse variance of flux
flux SPECTRA 1e-17 erg cm-2 s-1 AA-1 Coadded calibrated flux

Data Set: SDSS-DR16, AUX fields

Name Storage Units Description Default All
nspecobs AUX Number of spectroscopic observations of this source
nturnoff AUX Number of stars used for SNTURNOFF determination
objid AUX SDSS photometric object identification numbers (RUN, RERUN, CAMCOL, FIELD, ID)
plate AUX Plate number (each plate corresponds to an actual plug plate)
plateid AUX Unique database ID of plate based on PLATE, MJD, RUN2D (same as SkyServer version)
platequality AUX Final quality of plate this spectrum came from (good, marginal, or bad)
platerun AUX Drilling run that this plate was drilled in
platesn2 AUX Overall signal-to-noise-squared measure for plate (only for SDSS spectrograph plates)
primtarget AUX Target selection information at plate design, primary science selection (for backwards compatibility)
programname AUX Program within each survey that the plate was part of
rchi2 AUX Reduced chi-squared of best fit
rchi2diff AUX Difference in reduced chi-squared between best and second best fit
rchi2diff_noqso AUX Difference in reduced chi-squared between best and second best fit for Z_NOQSO redshift
run1d AUX Spectroscopic 1D reduction (redshift and classification) name
run2d AUX Spectroscopic 2D reduction (extraction of spectra) name
sectarget AUX Deprecated version of secondary (calibration) target flags (meanings highly overloaded)
segue1_target1 AUX Primary (science) target flags for SEGUE-1 targets
segue1_target2 AUX Primary (science) target flags for SEGUE-1 targets
segue2_target1 AUX Primary (science) target flags for SEGUE-2 targets
segue2_target2 AUX Secondary (calibration) target flags for SEGUE-2 targets
sn_median AUX Median signal-to-noise per pixel within each of the ugriz bandpasses
sn_median_all AUX Median signal-to-noise per pixel across full spectrum
snturnoff AUX Signal to noise measure for MS turnoff stars on plate (-9999 if not appropriate)
sourcetype AUX String expressing type of source (similar to OBJTYPE in DR8 and earlier)
spec1_g AUX Signal-to-noise squared for spectrograph #1, at g=20.20 for SDSS spectrograph spectra, g=21.20 for BOSS spectrograph spectra

Data Set: SDSS-DR16, SPECTRA fields

Name Storage Units Description Default All
flux SPECTRA 1e-17 erg cm-2 s-1 AA-1 Coadded calibrated flux
ivar SPECTRA 1e+34 cm4 s2 AA2 erg-2 Inverse variance of flux
mask SPECTRA and_mask
model SPECTRA 1e-17 erg cm-2 s-1 AA-1 Pipeline best model fit used for classification and redshift
sky SPECTRA 1e-17 erg cm-2 s-1 AA-1 Subtracted sky flux
wavelength SPECTRA AA Wavelength in units of Angstroms
wave_sigma SPECTRA pixel Line-spread function width (sigma of approximating Gaussian) in units of number of pixel

Data Set: SDSS-DR17-test, AUX fields

Name Storage Units Description Default All
elodie_dof AUX Degrees of freedom in fit to best ELODIE star
specsegue1 AUX Set to 1 for primary SDSS SEGUE-1 program observation of object, 0 otherwise
spec2_i AUX Signal-to-noise squared for spectrograph #2, at i=19.90 for SDSS spectrograph spectra, i=20.20 for BOSS spectrograph spectra
tile AUX Tile number (each tile can have several plates drilled for it)
rchi2diff_noqso AUX Difference in reduced chi-squared between best and second best fit for Z_NOQSO redshift
boss_target2 AUX Always set to zero (placeholder for BOSS target flags never used)
class_noqso AUX Spectroscopic classification for Z_NOQSO redshift
rchi2diff AUX Difference in reduced chi-squared between best and second best fit
elodie_logg AUX log10(gravity) of ELODIE star
elodie_bv AUX mag (B-V) color index for ELODIE star
segue2_target2 AUX Secondary (calibration) target flags for SEGUE-2 targets
snturnoff AUX Signal to noise measure for MS turnoff stars on plate (-9999 if not appropriate)
class_person AUX Visual-inspection classification (0=not inspected or unknown, 1=star, 2=narrow emission-line galaxy, 3=QSO, 4=galaxy)
thing_id_targeting AUX Resolve THING_ID in SDSS imaging for targeted object
npoly AUX Number of polynomial terms in fit
elodie_teff AUX Kelvin Effective temperature of ELODIE star
spec2_g AUX Signal-to-noise squared for spectrograph #2, at g=20.20 for SDSS spectrograph spectra, g=21.20 for BOSS spectrograph spectra
fluxobjid AUX Unique database ID of flux-based photometric match based on RUN, RERUN, CAMCOl, FIELD, ID (same as SkyServer version)
vdispchi2 AUX Chi-squared for best-fit velocity dispersion
anyormask AUX For each bit, records whether any pixel in the spectrum has that bit set in its ORMASK
spectroflux_ivar AUX nanomaggy-2 Inverse variance of spectrum projected onto ugriz filters
plate AUX Plate number (each plate corresponds to an actual plug plate)
marvels_target1 AUX Primary (science) target flags for MARVELS targets
boss_specobj_id AUX Identification number internal to BOSS for SPECBOSS=1 objects
cz AUX z of Normal unit vector in J2000

Data Set: SDSS-DR17-test, SPECTRA fields

Name Storage Units Description Default All
flux SPECTRA 1e-17 erg cm-2 s-1 AA-1 Coadded calibrated flux
ivar SPECTRA 1e+34 cm4 s2 AA2 erg-2 Inverse variance of flux
mask SPECTRA and_mask
model SPECTRA 1e-17 erg cm-2 s-1 AA-1 Pipeline best model fit used for classification and redshift
sky SPECTRA 1e-17 erg cm-2 s-1 AA-1 Subtracted sky flux
wavelength SPECTRA AA Wavelength in units of Angstroms
wave_sigma SPECTRA pixel Line-spread function width (sigma of approximating Gaussian) in units of number of pixel

Data Set: DESI-EDR, AUX fields

Name Storage Units Description Default All
tsnr2_gpbdark AUX GPBDARK template (S/N)^2 summed over BRZ
sv_primary AUX Boolean flag (True/False) for the primary coadded spectrum in SV (SV1+2+3)
sv3_desi_target AUX DESI (dark time program) target selection bitmask for SV3
tsnr2_gpbbackup AUX GPBBACKUP template (S/N)^2 summed over BRZ
survey AUX Survey name
sv3_mws_target AUX MWS (bright time program) target selection bitmask for SV3
zcat_nspec AUX Number of coadded spectra for this TARGETID in this zcatalog
desi_target AUX DESI (dark time program) target selection bitmask
ncoeff AUX Number of Redrock template coefficients
npixels AUX Number of unmasked wavelengths that contributed to the redshift fit
mean_delta_y AUX mm Mean (over exposures) fiber difference requested - actual CS5 Y location on focal plane
mean_fiber_ra AUX deg Mean (over exposures) RA of actual fiber position
lastnight AUX Last calendar date of the exposures used in the coadded spectrum as YYYYMMDD of the beginning of the observing night
mean_fiber_dec AUX deg Mean (over exposures) DEC of actual fiber position
firstnight AUX First calendar date of the exposures used in the coadded spectrum as YYYYMMDD of the beginning of the observing night
mean_mjd AUX days Mean (over exposures) of the Modified Julian Date (MJD) when the shutter was opened

Data Set: DESI-EDR, SPECTRA fields

Name Storage Units Description Default All
flux SPECTRA 1e-17 erg cm-2 s-1 AA-1 Coadded calibrated flux
ivar SPECTRA 1e+34 cm4 s2 AA2 erg-2 Inverse variance of flux
mask SPECTRA Mask value
model SPECTRA 1e-17 erg cm-2 s-1 AA-1 Pipeline best model fit
wavelength SPECTRA AA Wavelength in units of Angstroms
wave_sigma SPECTRA AA Line-spread function width (sigma of approximating Gaussian) in units of Angstroms
SPARCL Field Cat(alog)