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
file CORE File used for this record
dateobs CORE Range of observational dates for a given spectrum (single value for a single date)
redshift_warning CORE Bitmask with warning on redshift result
dateobs_center CORE Central value of the dateobs range
updated CORE Date and time when the record was created/updated
site CORE [Categorical] Site of observations
datasetgroup CORE [Categorical] Common name for a coherent set of spectra published as a single release (e.g., SDSS_BOSS)
redshift_err CORE Uncertainty on the measured redshift, or radial velocity in units of redshift
wavemax CORE AA Maximum value of wavelength coverage in Angstroms
extra_files CORE Additional files read for ingest
exptime CORE second Exposure time in seconds
instrument CORE [Categorical] Instrument used for observation
redshift CORE Measured redshift, or radial velocity in units of redshift
targetid CORE Dataset-specific photometric target identifier
specprimary CORE Whether an entry is the primary spectrum for a given target object
data_release CORE [Categorical] Data release of a given record (with a common data structure, e.g., SDSS-DR16, BOSS-DR16)
wavemin CORE AA Minimum value of wavelength coverage in Angstroms
spectype CORE [Categorical] Spectral type of the object (STAR, GALAXY, QSO)
telescope CORE [Categorical] Telescope used for the observation
specid CORE Dataset-specific spectrum identifier (may not be unique)
sparcl_id CORE Universally Unique Identifier for spectrum in SPARCL
dec CORE deg Declination in degrees
ra CORE deg Right Ascension in degrees
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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
snturnoff AUX Signal to noise measure for MS turnoff stars on plate (-9999 if not appropriate)
thing_id AUX Resolve THING_ID in SDSS imaging for best positional match
sn_median AUX Median signal-to-noise per pixel within each of the ugriz bandpasses
zoffset AUX micron Washer thickness used for backstopping BOSS quasar targets, so they are closer to 4000 Angstrom focal plan
elodie_logg AUX log10(gravity) of ELODIE star
fiberid AUX Fiber number
spec2_r AUX Signal-to-noise squared for spectrograph #2, at r=20.25 for SDSS spectrograph spectra, r=20.20 for BOSS spectrograph spectra
vdisp_err AUX km s-1 Error in velocity dispersion
run2d AUX Spectroscopic 2D reduction (extraction of spectra) name
designid AUX Design identification number for plate
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
wcoverage AUX Coverage in wavelength, in units of log10 wavelength
fracnsigma AUX Fraction of pixels deviant by more than N sigma relative to best-fit (for 1,2,..,10 sigma)
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
special_target2 AUX Secondary (calibration) target flags for SDSS-I and SDSS-II special program targets
z_err_noqso AUX Error in Z_NOQSO redshift
spec1_r AUX Signal-to-noise squared for spectrograph #1, at r=20.25 for SDSS spectrograph spectra, r=20.20 for BOSS spectrograph spectra
nturnoff AUX Number of stars used for SNTURNOFF determination
elodie_z_modelerr AUX Standard deviation in Elodie redshift among the 12 best-fit stars
survey AUX Survey name

Data Set: BOSS-DR16, SPECTRA fields

Name Storage Units Description Default All
sky SPECTRA 1e-17 erg cm-2 s-1 AA-1 Subtracted sky flux
flux SPECTRA 1e-17 erg cm-2 s-1 AA-1 Coadded calibrated flux
model SPECTRA 1e-17 erg cm-2 s-1 AA-1 Pipeline best model fit used for classification and redshift
ivar SPECTRA 1e+34 cm4 s2 AA2 erg-2 Inverse variance of 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
mask SPECTRA and_mask

Data Set: SDSS-DR16, AUX fields

Name Storage Units Description Default All
lambda_eff AUX AA Effective wavelength drilling position was optimized for
mjd AUX days Modified Julian Day of observation
elodie_teff AUX Kelvin Effective temperature of ELODIE star
vdisp AUX km s-1 Velocity dispersion
vdisp_err AUX km s-1 Error in velocity dispersion
elodie_bv AUX mag (B-V) color index for ELODIE star
zoffset AUX micron Washer thickness used for backstopping BOSS quasar targets, so they are closer to 4000 Angstrom focal plan
yfocal AUX mm Hole position on plate (+Y = +DEC)
xfocal AUX mm Hole position on plate (+X = +RA)
calibflux AUX nanomaggy ugriz fluxes used for calibrations
spectroflux AUX nanomaggy Spectrum projected onto ugriz filters
spectrosynflux AUX nanomaggy Best-fit template spectrum projected onto ugriz filters
spectroskyflux AUX nanomaggy Sky flux in each of the ugriz imaging filters
spectroflux_ivar AUX nanomaggy-2 Inverse variance of spectrum projected onto ugriz filters
spectrosynflux_ivar AUX nanomaggy-2 Inverse variance of best-fit template spectrum projected onto ugriz filters
calibflux_ivar AUX nanomaggy-2 Inverse variances of ugriz fluxes used for calibrations
cz AUX z of Normal unit vector in J2000
special_target2 AUX Secondary (calibration) target flags for SDSS-I and SDSS-II special program targets
eboss_target_id AUX EBOSS unique target identifier for every spectroscopic target
thing_id AUX Resolve THING_ID in SDSS imaging for best positional match
run1d AUX Spectroscopic 1D reduction (redshift and classification) name
targetobjid AUX Unique database ID of targeting object based on RUN, RERUN, CAMCOl, FIELD, ID (same as SkyServer version)
targettype AUX General type of target (SCIENCE, STANDARD, or SKY)
legacy_target2 AUX Secondary (calibration) target flags for SDSS-I and SDSS-II Legacy survey
spectrographid AUX Which spectrograph (1 or 2)

Data Set: SDSS-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
sky SPECTRA 1e-17 erg cm-2 s-1 AA-1 Subtracted sky 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
flux SPECTRA 1e-17 erg cm-2 s-1 AA-1 Coadded calibrated flux
wavelength SPECTRA AA Wavelength in units of Angstroms

Data Set: SDSS-DR17-test, AUX fields

Name Storage Units Description Default All
sourcetype AUX String expressing type of source (similar to OBJTYPE in DR8 and earlier)
survey AUX Survey name
primtarget AUX Target selection information at plate design, primary science selection (for backwards compatibility)
theta AUX Template coefficients of best fit
tile AUX Tile number (each tile can have several plates drilled for it)
calibflux AUX nanomaggy ugriz fluxes used for calibrations
fluxobjid AUX Unique database ID of flux-based photometric match based on RUN, RERUN, CAMCOl, FIELD, ID (same as SkyServer version)
plateid AUX Unique database ID of plate based on PLATE, MJD, RUN2D (same as SkyServer version)
targetobjid AUX Unique database ID of targeting object based on RUN, RERUN, CAMCOl, FIELD, ID (same as SkyServer version)
vdisp AUX km s-1 Velocity dispersion
class_person AUX Visual-inspection classification (0=not inspected or unknown, 1=star, 2=narrow emission-line galaxy, 3=QSO, 4=galaxy)
comments_person AUX Visual-inspection comments
z_conf_person AUX Visual-inspection confidence (0=not inspected or no confidence, 1,2=low confidence, 3,4=high confidence)
z_person AUX Visual-inspection redshift
zwarning_noqso AUX Warnings in z_noqso redshift (BOSS spectra only)
zoffset AUX micron Washer thickness used for backstopping BOSS quasar targets, so they are closer to 4000 Angstrom focal plan
spectrographid AUX Which spectrograph (1 or 2)
cx AUX x of Normal unit vector in J2000
cy AUX y of Normal unit vector in J2000
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
bgs_target AUX BGS (Bright Galaxy Survey) target selection bitmask
chi2 AUX Best fit chi-squared
cmx_target AUX Target selection bitmask for commissioning
coadd_fiberstatus AUX Bitwise AND of the FIBERSTATUS values of the spectra used in the coadd
coadd_numexp AUX Number of exposures included in the coadd for this target
coadd_numnight AUX Number of different nights included in the coadd for this target
coadd_numtile AUX Number of different tiles included in the coadd for this target
coeff AUX Redrock template coefficients
deltachi2 AUX Delta-chi-squared for template fit from Redrock
desi_target AUX DESI (dark time program) target selection bitmask
fa_target AUX Targeting bit internally used by fiberassign (linked with FA_TYPE)
fa_type AUX Fiberassign internal target type (science, standard, sky, safe, suppsky)
firstnight AUX First calendar date of the exposures used in the coadded spectrum as YYYYMMDD of the beginning of the observing night
healpix AUX HEALPixel containing this location at NSIDE=64 in the NESTED scheme
lastnight AUX Last calendar date of the exposures used in the coadded spectrum as YYYYMMDD of the beginning of the observing night
mean_delta_x AUX mm Mean (over exposures) fiber difference between measured and requested CS5 X location on focal plane
mean_delta_y AUX mm Mean (over exposures) fiber difference requested - actual CS5 Y location on focal plane
mean_fiber_dec AUX deg Mean (over exposures) DEC of actual fiber position
mean_fiber_ra AUX deg Mean (over exposures) RA of actual fiber position
mean_mjd AUX days Mean (over exposures) of the Modified Julian Date (MJD) when the shutter was opened
mean_psf_to_fiber_specflux AUX Mean of input exposures fraction of light from point-like source captured by 1.5 arcsec diameter fiber given atmospheric seeing
mws_target AUX Milky Way Survey targeting bits
ncoeff AUX Number of Redrock template coefficients
npixels AUX Number of unmasked wavelengths that contributed to the redshift fit
numobs_init AUX Initial number of observations for target calculated across target selection bitmasks and OBSCONDITIONS

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)