DES DR2 Main (des_dr2.main)
The table has 691483608 rows, 215 columns.
Description
(paragraph adapted from the DES DR2 paper)
"DR2_MAIN includes all the main quantities extracted from the coadd pipeline and important information about the objects. That table also includes MAG_AUTO and WAVG_MAG_PSF, associated uncertainties, as well as the corresponding dereddened magnitudes along with star/galaxy separation columns."
Reference
Find details about DES and its second data release on:
Attribution
This project used public archival data from the Dark Energy Survey (DES). Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana–Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico and the Ministério da Ciência, Tecnologia e Inovação, the Deutsche Forschungsgemeinschaft and the Collaborating Institutions in the Dark Energy Survey.
The Collaborating Institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones Enérgeticas, Medioambientales y Tecnológicas–Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgenössische Technische Hochschule (ETH) Zürich, Fermi National Accelerator Laboratory, the University of Illinois at Urbana-Champaign, the Institut de Ciències de l'Espai (IEEC/CSIC), the Institut de Física d'Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universität München and the associated Excellence Cluster Universe, the University of Michigan, the National Optical Astronomy Observatory, the University of Nottingham, the Ohio State University, the OzDES Membership Consortium, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the University of Sussex, and Texas A&M University.
Based in part on observations at Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, which is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation.
Database access and other data services are provided by the Associação Laboratório Interinstitucional de e-Astronomia (LIneA) with the financial support from INCT do e-Universo (Processo n.º 465376/2014-2).
Columns
Name | Type | UCD | Unit | Description |
---|---|---|---|---|
coadd_object_id | long |
meta.id meta.main |
Unique identifier for the coadded objects |
|
tilename | char | obs.field |
Identifier of each one of the tiles on which the survey is gridded |
|
hpix_32 | long |
pos.healpix phys.size |
Healpix identifier for its 32 grid size, in a NESTED schema |
|
hpix_64 | long |
pos.healpix phys.size |
Healpix identifier for its 64 grid size, in a NESTED schema |
|
hpix_1024 | long |
pos.healpix phys.size |
Healpix identifier for its 1024 grid size, in a NESTED schema |
|
hpix_4096 | long |
pos.healpix phys.size |
Healpix identifier for its 4096 grid size, in a NESTED schema |
|
hpix_16384 | long |
pos.healpix phys.size |
Healpix identifier for its 16384 grid size, in a NESTED schema |
|
ra | double | pos.eq.ra | deg |
Right ascension, with quantized precision for indexing (DELTAWIN_J2000 has full precision but not indexed) |
dec | double | pos.eq.dec | deg |
decl., with quantized precision for indexing (DELTAWIN_J2000 has full precision but not indexed) |
alphawin_j2000 | double | pos.eq.ra | deg |
Right ascension for the object, J2000 in ICRS system (full precision but not indexed) |
deltawin_j2000 | double | pos.eq.dec | deg |
decl. for the object, J2000 in ICRS system (full precision but not indexed) |
galactic_l | double | pos.galactic.lon | deg |
Galactic Longitud |
galactic_b | double | pos.galactic.lat | deg |
Galactic Latitude |
xwin_image | double | obs.image | pixel |
X-centroid from windowed measurements on coadded image |
ywin_image | double | obs.image | pixel |
Y-centroid from windowed measurements on coadded image |
a_image | double |
phys.angSize phys.size.diameter phys.size |
pixel |
Major axis size based on an isophotal model |
erra_image | double |
phys.angSize phys.size.diameter phys.size |
pixel |
Uncertainty in major axis size, from isophotal model |
b_image | double |
phys.angSize phys.size meta.modelled |
pixel |
Minor axis size based on an isophotal model |
errb_image | double |
phys.angSize phys.size meta.modelled |
pixel |
Uncertainty in minor axis size, from isophotal model |
theta_j2000 | double |
pos.posAng pos phys.angSize |
deg |
Position angle of source in J2000 coordinates, from nonwindowed measurement |
errtheta_image | double |
meta.code.error meta.modelled src |
deg |
Uncertainty in source position, from isophotal model |
kron_radius | double |
phys.size.radius instr.sensitivity |
pixel |
Kron radius measured from detection image |
ebv_sfd98 | double |
phot.color em.opt.V em.opt.B |
mag |
E(B-V) reddening coefficient from Schlegel, Finkbeiner & Davis, 1998 |
mag_auto_g_dered | double |
phot.mag.reddFree meta.modelled phys.size.radius |
mag |
Dereddened magnitude estimation (using SFD98), for an elliptical model based on the Kron radius |
mag_auto_r_dered | double |
phot.mag.reddFree meta.modelled phys.size.radius |
mag |
Dereddened magnitude estimation (using SFD98), for an elliptical model based on the Kron radius |
mag_auto_i_dered | double |
phot.mag.reddFree meta.modelled phys.size.radius |
mag |
Dereddened magnitude estimation (using SFD98), for an elliptical model based on the Kron radius |
mag_auto_z_dered | double |
phot.mag.reddFree meta.modelled phys.size.radius |
mag |
Dereddened magnitude estimation (using SFD98), for an elliptical model based on the Kron radius |
mag_auto_y_dered | double |
phot.mag.reddFree meta.modelled phys.size.radius |
mag |
Dereddened magnitude estimation (using SFD98), for an elliptical model based on the Kron radius |
wavg_mag_psf_g_dered | double |
phot.mag.reddFree instr.det.psf phot.mag |
mag |
Dereddened weighted-average magnitude (using SFD98) from PSF fit single-epoch detections |
wavg_mag_psf_r_dered | double |
phot.mag.reddFree instr.det.psf phot.mag |
mag |
Dereddened weighted-average magnitude (using SFD98) from PSF fit single-epoch detections |
wavg_mag_psf_i_dered | double |
phot.mag.reddFree instr.det.psf phot.mag |
mag |
Dereddened weighted-average magnitude (using SFD98) from PSF fit single-epoch detections |
wavg_mag_psf_z_dered | double |
phot.mag.reddFree instr.det.psf phot.mag |
mag |
Dereddened weighted-average magnitude (using SFD98) from PSF fit single-epoch detections |
wavg_mag_psf_y_dered | double |
phot.mag.reddFree instr.det.psf phot.mag |
mag |
Dereddened weighted-average magnitude (using SFD98) from PSF fit single-epoch detections |
extended_class_coadd | int |
src.class.starGalaxy meta.checksum phot |
0: high-confidence stars; 1: candidate stars; 2: mostly gxs; 3: high-confidence gxs; -9: No data; Sextractor photometry |
|
extended_class_wavg | int |
src.class.starGalaxy meta.checksum phot |
0: high-confidence stars; 1: candidate stars; 2: mostly gxs; 3: high-confidence gxs; -9: No data; WAVG photometry |
|
flags_g | int |
meta.code src |
Flag describing cautionary advice about source extraction process (FLAGS < 4 for well-behaved objects) |
|
imaflags_iso_g | int |
meta.code instr.pixel obs.image |
Flag identifying sources with missing/flagged pixels, considering all single-epoch images |
|
nepochs_g | int | time.epoch |
Number of epochs the source is detected in single-epoch images |
|
flags_r | int |
meta.code src |
Flag describing cautionary advice about source extraction process (FLAGS < 4 for well-behaved objects) |
|
imaflags_iso_r | int |
meta.code instr.pixel obs.image |
Flag identifying sources with missing/flagged pixels, considering all single-epoch images |
|
nepochs_r | int | time.epoch |
Number of epochs the source is detected in single-epoch images |
|
flags_i | int |
meta.code src |
Flag describing cautionary advice about source extraction process (FLAGS < 4 for well-behaved objects) |
|
imaflags_iso_i | int |
meta.code instr.pixel obs.image |
Flag identifying sources with missing/flagged pixels, considering all single-epoch images |
|
nepochs_i | int | time.epoch |
Number of epochs the source is detected in single-epoch images |
|
flags_z | int |
meta.code src |
Flag describing cautionary advice about source extraction process (FLAGS < 4 for well-behaved objects) |
|
imaflags_iso_z | int |
meta.code instr.pixel obs.image |
Flag identifying sources with missing/flagged pixels, considering all single-epoch images |
|
nepochs_z | int | time.epoch |
Number of epochs the source is detected in single-epoch images |
|
flags_y | int |
meta.code src |
Flag describing cautionary advice about source extraction process (FLAGS < 4 for well-behaved objects) |
|
imaflags_iso_y | int |
meta.code instr.pixel obs.image |
Flag identifying sources with missing/flagged pixels, considering all single-epoch images |
|
nepochs_y | int | time.epoch |
Number of epochs the source is detected in single-epoch images |
|
xwin_image_g | double |
instr.bandpass obs.image |
pixel |
X-centroid from windowed measurements on coadded band image |
xwin_image_r | double |
instr.bandpass obs.image |
pixel |
X-centroid from windowed measurements on coadded band image |
xwin_image_i | double |
instr.bandpass obs.image |
pixel |
X-centroid from windowed measurements on coadded band image |
xwin_image_z | double |
instr.bandpass obs.image |
pixel |
X-centroid from windowed measurements on coadded band image |
xwin_image_y | double |
instr.bandpass obs.image |
pixel |
X-centroid from windowed measurements on coadded band image |
ywin_image_g | double |
instr.bandpass obs.image |
pixel |
Y-centroid from windowed measurements on coadded band images |
ywin_image_r | double |
instr.bandpass obs.image |
pixel |
Y-centroid from windowed measurements on coadded band images |
ywin_image_i | double |
instr.bandpass obs.image |
pixel |
Y-centroid from windowed measurements on coadded band images |
ywin_image_z | double |
instr.bandpass obs.image |
pixel |
Y-centroid from windowed measurements on coadded band images |
ywin_image_y | double |
instr.bandpass obs.image |
pixel |
Y-centroid from windowed measurements on coadded band images |
x2win_image_g | double | time.duration | pixel² |
Second moment in x-direction, from converged windowed measurements |
x2win_image_r | double | time.duration | pixel² |
Second moment in x-direction, from converged windowed measurements |
x2win_image_i | double | time.duration | pixel² |
Second moment in x-direction, from converged windowed measurements |
x2win_image_z | double | time.duration | pixel² |
Second moment in x-direction, from converged windowed measurements |
x2win_image_y | double | time.duration | pixel² |
Second moment in x-direction, from converged windowed measurements |
y2win_image_g | double | time.duration | pixel² |
Second moment in y-direction, from converged windowed measurements |
y2win_image_r | double | time.duration | pixel² |
Second moment in y-direction, from converged windowed measurements |
y2win_image_i | double | time.duration | pixel² |
Second moment in y-direction, from converged windowed measurements |
y2win_image_z | double | time.duration | pixel² |
Second moment in y-direction, from converged windowed measurements |
y2win_image_y | double | time.duration | pixel² |
Second moment in y-direction, from converged windowed measurements |
xywin_image_g | double | time.duration | pixel² |
Second moment in xy-direction, from converged windowed measurements |
xywin_image_r | double | time.duration | pixel² |
Second moment in xy-direction, from converged windowed measurements |
xywin_image_i | double | time.duration | pixel² |
Second moment in xy-direction, from converged windowed measurements |
xywin_image_z | double | time.duration | pixel² |
Second moment in xy-direction, from converged windowed measurements |
xywin_image_y | double | time.duration | pixel² |
Second moment in xy-direction, from converged windowed measurements |
errx2win_image_g | double |
meta.code.error pos.centroid |
pixel² |
Uncertainty in second moment of x-distribution centroid, from converged windowed measurements |
errx2win_image_r | double |
meta.code.error pos.centroid |
pixel² |
Uncertainty in second moment of x-distribution centroid, from converged windowed measurements |
errx2win_image_i | double |
meta.code.error pos.centroid |
pixel² |
Uncertainty in second moment of x-distribution centroid, from converged windowed measurements |
errx2win_image_z | double |
meta.code.error pos.centroid |
pixel² |
Uncertainty in second moment of x-distribution centroid, from converged windowed measurements |
errx2win_image_y | double |
meta.code.error pos.centroid |
pixel² |
Uncertainty in second moment of x-distribution centroid, from converged windowed measurements |
erry2win_image_g | double |
meta.code.error pos.centroid |
pixel² |
Uncertainty in second moment of y-distribution centroid, from converged windowed measurements |
erry2win_image_r | double |
meta.code.error pos.centroid |
pixel² |
Uncertainty in second moment of y-distribution centroid, from converged windowed measurements |
erry2win_image_i | double |
meta.code.error pos.centroid |
pixel² |
Uncertainty in second moment of y-distribution centroid, from converged windowed measurements |
erry2win_image_z | double |
meta.code.error pos.centroid |
pixel² |
Uncertainty in second moment of y-distribution centroid, from converged windowed measurements |
erry2win_image_y | double |
meta.code.error pos.centroid |
pixel² |
Uncertainty in second moment of y-distribution centroid, from converged windowed measurements |
errxywin_image_g | double | meta.code.error | pixel² |
Uncertainty in second moment of xy-distribution, from converged windowed measurements |
errxywin_image_r | double | meta.code.error | pixel² |
Uncertainty in second moment of xy-distribution, from converged windowed measurements |
errxywin_image_i | double | meta.code.error | pixel² |
Uncertainty in second moment of xy-distribution, from converged windowed measurements |
errxywin_image_z | double | meta.code.error | pixel² |
Uncertainty in second moment of xy-distribution, from converged windowed measurements |
errxywin_image_y | double | meta.code.error | pixel² |
Uncertainty in second moment of xy-distribution, from converged windowed measurements |
awin_image_g | double |
phys.angSize phys.size.diameter phys.size |
pixel |
Major axis size, from 2nd order windowed moment measurements |
awin_image_r | double |
phys.angSize phys.size.diameter phys.size |
pixel |
Major axis size, from 2nd order windowed moment measurements |
awin_image_i | double |
phys.angSize phys.size.diameter phys.size |
pixel |
Major axis size, from 2nd order windowed moment measurements |
awin_image_z | double |
phys.angSize phys.size.diameter phys.size |
pixel |
Major axis size, from 2nd order windowed moment measurements |
awin_image_y | double |
phys.angSize phys.size.diameter phys.size |
pixel |
Major axis size, from 2nd order windowed moment measurements |
bwin_image_g | double |
phys.angSize phys.size |
pixel |
Minor axis size, from 2nd order windowed moment measurements |
bwin_image_r | double |
phys.angSize phys.size |
pixel |
Minor axis size, from 2nd order windowed moment measurements |
bwin_image_i | double |
phys.angSize phys.size |
pixel |
Minor axis size, from 2nd order windowed moment measurements |
bwin_image_z | double |
phys.angSize phys.size |
pixel |
Minor axis size, from 2nd order windowed moment measurements |
bwin_image_y | double |
phys.angSize phys.size |
pixel |
Minor axis size, from 2nd order windowed moment measurements |
thetawin_image_g | double |
pos.cartesian.x pos.cartesian.y pos.posAng |
deg |
Position angle of source, for converged windowed measurement grow from x to y |
thetawin_image_r | double |
pos.cartesian.x pos.cartesian.y pos.posAng |
deg |
Position angle of source, for converged windowed measurement grow from x to y |
thetawin_image_i | double |
pos.cartesian.x pos.cartesian.y pos.posAng |
deg |
Position angle of source, for converged windowed measurement grow from x to y |
thetawin_image_z | double |
pos.cartesian.x pos.cartesian.y pos.posAng |
deg |
Position angle of source, for converged windowed measurement grow from x to y |
thetawin_image_y | double |
pos.cartesian.x pos.cartesian.y pos.posAng |
deg |
Position angle of source, for converged windowed measurement grow from x to y |
errawin_image_g | double |
phys.angSize phys.size.diameter phys.size |
pixel |
Uncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noise |
errawin_image_r | double |
phys.angSize phys.size.diameter phys.size |
pixel |
Uncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noise |
errawin_image_i | double |
phys.angSize phys.size.diameter phys.size |
pixel |
Uncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noise |
errawin_image_z | double |
phys.angSize phys.size.diameter phys.size |
pixel |
Uncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noise |
errawin_image_y | double |
phys.angSize phys.size.diameter phys.size |
pixel |
Uncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noise |
errbwin_image_g | double |
phys.angSize phys.size instr.det.noise |
pixel |
Uncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noise |
errbwin_image_r | double |
phys.angSize phys.size instr.det.noise |
pixel |
Uncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noise |
errbwin_image_i | double |
phys.angSize phys.size instr.det.noise |
pixel |
Uncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noise |
errbwin_image_z | double |
phys.angSize phys.size instr.det.noise |
pixel |
Uncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noise |
errbwin_image_y | double |
phys.angSize phys.size instr.det.noise |
pixel |
Uncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noise |
errthetawin_image_g | double |
pos.posAng phys.angSize |
deg |
Uncertainty in source position angle, from converged windowed measurement |
errthetawin_image_r | double |
pos.posAng phys.angSize |
deg |
Uncertainty in source position angle, from converged windowed measurement |
errthetawin_image_i | double |
pos.posAng phys.angSize |
deg |
Uncertainty in source position angle, from converged windowed measurement |
errthetawin_image_z | double |
pos.posAng phys.angSize |
deg |
Uncertainty in source position angle, from converged windowed measurement |
errthetawin_image_y | double |
pos.posAng phys.angSize |
deg |
Uncertainty in source position angle, from converged windowed measurement |
flux_radius_g | double |
phys.size.radius meta.modelled |
pixel |
Half-light radius for the object, from elliptical growth-curve, modeled in two-dimensions |
flux_radius_r | double |
phys.size.radius meta.modelled |
pixel |
Half-light radius for the object, from elliptical growth-curve, modeled in two-dimensions |
flux_radius_i | double |
phys.size.radius meta.modelled |
pixel |
Half-light radius for the object, from elliptical growth-curve, modeled in two-dimensions |
flux_radius_z | double |
phys.size.radius meta.modelled |
pixel |
Half-light radius for the object, from elliptical growth-curve, modeled in two-dimensions |
flux_radius_y | double |
phys.size.radius meta.modelled |
pixel |
Half-light radius for the object, from elliptical growth-curve, modeled in two-dimensions |
fwhm_image_g | double |
spect.line.width stat.fwhm |
pixel |
FWHM measured from the isophotal area, from elliptical growth-curve, modeled in two-dimensions |
fwhm_image_r | double |
spect.line.width stat.fwhm |
pixel |
FWHM measured from the isophotal area, from elliptical growth-curve, modeled in two-dimensions |
fwhm_image_i | double |
spect.line.width stat.fwhm |
pixel |
FWHM measured from the isophotal area, from elliptical growth-curve, modeled in two-dimensions |
fwhm_image_z | double |
spect.line.width stat.fwhm |
pixel |
FWHM measured from the isophotal area, from elliptical growth-curve, modeled in two-dimensions |
fwhm_image_y | double |
spect.line.width stat.fwhm |
pixel |
FWHM measured from the isophotal area, from elliptical growth-curve, modeled in two-dimensions |
isoarea_image_g | int |
meta.ref phys.angArea phys.area |
pixel² |
Isophotal area of the coadded source |
isoarea_image_r | int |
meta.ref phys.angArea phys.area |
pixel² |
Isophotal area of the coadded source |
isoarea_image_i | int |
meta.ref phys.angArea phys.area |
pixel² |
Isophotal area of the coadded source |
isoarea_image_z | int |
meta.ref phys.angArea phys.area |
pixel² |
Isophotal area of the coadded source |
isoarea_image_y | int |
meta.ref phys.angArea phys.area |
pixel² |
Isophotal area of the coadded source |
background_g | double |
instr.background phys.atmol.level src.net |
mag |
Background level, by CCD-amplifier |
background_r | double |
instr.background phys.atmol.level src.net |
mag |
Background level, by CCD-amplifier |
background_i | double |
instr.background phys.atmol.level src.net |
mag |
Background level, by CCD-amplifier |
background_z | double |
instr.background phys.atmol.level src.net |
mag |
Background level, by CCD-amplifier |
background_y | double |
instr.background phys.atmol.level src.net |
mag |
Background level, by CCD-amplifier |
niter_model_g | int |
meta.id meta.modelled phot |
Number of iterations in model fitting photometric measurements |
|
niter_model_r | int |
meta.id meta.modelled phot |
Number of iterations in model fitting photometric measurements |
|
niter_model_i | int |
meta.id meta.modelled phot |
Number of iterations in model fitting photometric measurements |
|
niter_model_z | int |
meta.id meta.modelled phot |
Number of iterations in model fitting photometric measurements |
|
niter_model_y | int |
meta.id meta.modelled phot |
Number of iterations in model fitting photometric measurements |
|
kron_radius_g | double |
phys.size.radius obs.image |
pixel |
Kron radius measured from coadded image |
kron_radius_r | double |
phys.size.radius obs.image |
pixel |
Kron radius measured from coadded image |
kron_radius_i | double |
phys.size.radius obs.image |
pixel |
Kron radius measured from coadded image |
kron_radius_z | double |
phys.size.radius obs.image |
pixel |
Kron radius measured from coadded image |
kron_radius_y | double |
phys.size.radius obs.image |
pixel |
Kron radius measured from coadded image |
mag_auto_g | double |
phys.size.radius meta.modelled |
mag |
Magnitude estimation, for an elliptical model based on the Kron radius |
mag_auto_r | double |
phys.size.radius meta.modelled |
mag |
Magnitude estimation, for an elliptical model based on the Kron radius |
mag_auto_i | double |
phys.size.radius meta.modelled |
mag |
Magnitude estimation, for an elliptical model based on the Kron radius |
mag_auto_z | double |
phys.size.radius meta.modelled |
mag |
Magnitude estimation, for an elliptical model based on the Kron radius |
mag_auto_y | double |
phys.size.radius meta.modelled |
mag |
Magnitude estimation, for an elliptical model based on the Kron radius |
magerr_auto_g | double |
meta.code.error meta.modelled phys.size.radius |
mag |
Uncertainty in magnitude estimation, for an elliptical model based on the Kron radius |
magerr_auto_r | double |
meta.code.error meta.modelled phys.size.radius |
mag |
Uncertainty in magnitude estimation, for an elliptical model based on the Kron radius |
magerr_auto_i | double |
meta.code.error meta.modelled phys.size.radius |
mag |
Uncertainty in magnitude estimation, for an elliptical model based on the Kron radius |
magerr_auto_z | double |
meta.code.error meta.modelled phys.size.radius |
mag |
Uncertainty in magnitude estimation, for an elliptical model based on the Kron radius |
magerr_auto_y | double |
meta.code.error meta.modelled phys.size.radius |
mag |
Uncertainty in magnitude estimation, for an elliptical model based on the Kron radius |
wavg_mag_psf_g | double |
phot.mag instr.det.psf instr.sensitivity |
mag |
Weighted-average magnitude, of PSF fit single-epoch detections |
wavg_mag_psf_r | double |
phot.mag instr.det.psf instr.sensitivity |
mag |
Weighted-average magnitude, of PSF fit single-epoch detections |
wavg_mag_psf_i | double |
phot.mag instr.det.psf instr.sensitivity |
mag |
Weighted-average magnitude, of PSF fit single-epoch detections |
wavg_mag_psf_z | double |
phot.mag instr.det.psf instr.sensitivity |
mag |
Weighted-average magnitude, of PSF fit single-epoch detections |
wavg_mag_psf_y | double |
phot.mag instr.det.psf instr.sensitivity |
mag |
Weighted-average magnitude, of PSF fit single-epoch detections |
wavg_magerr_psf_g | double |
meta.code.error instr.det.psf phot.mag |
mag |
Uncertainty of weighted averaged magnitude, of PSF fit single-epoch detections |
wavg_magerr_psf_r | double |
meta.code.error instr.det.psf phot.mag |
mag |
Uncertainty of weighted averaged magnitude, of PSF fit single-epoch detections |
wavg_magerr_psf_i | double |
meta.code.error instr.det.psf phot.mag |
mag |
Uncertainty of weighted averaged magnitude, of PSF fit single-epoch detections |
wavg_magerr_psf_z | double |
meta.code.error instr.det.psf phot.mag |
mag |
Uncertainty of weighted averaged magnitude, of PSF fit single-epoch detections |
wavg_magerr_psf_y | double |
meta.code.error instr.det.psf phot.mag |
mag |
Uncertainty of weighted averaged magnitude, of PSF fit single-epoch detections |
flux_auto_g | double |
phys.size.radius meta.modelled |
ADU |
Aperture-flux measurement, elliptical model based on the Kron radius |
flux_auto_r | double |
phys.size.radius meta.modelled |
ADU |
Aperture-flux measurement, elliptical model based on the Kron radius |
flux_auto_i | double |
phys.size.radius meta.modelled |
ADU |
Aperture-flux measurement, elliptical model based on the Kron radius |
flux_auto_z | double |
phys.size.radius meta.modelled |
ADU |
Aperture-flux measurement, elliptical model based on the Kron radius |
flux_auto_y | double |
phys.size.radius meta.modelled |
ADU |
Aperture-flux measurement, elliptical model based on the Kron radius |
fluxerr_auto_g | double |
meta.code.error meta.modelled phys.size.radius |
ADU |
Uncertainty in aperture-flux measurement, elliptical model based on the Kron radius |
fluxerr_auto_r | double |
meta.code.error meta.modelled phys.size.radius |
ADU |
Uncertainty in aperture-flux measurement, elliptical model based on the Kron radius |
fluxerr_auto_i | double |
meta.code.error meta.modelled phys.size.radius |
ADU |
Uncertainty in aperture-flux measurement, elliptical model based on the Kron radius |
fluxerr_auto_z | double |
meta.code.error meta.modelled phys.size.radius |
ADU |
Uncertainty in aperture-flux measurement, elliptical model based on the Kron radius |
fluxerr_auto_y | double |
meta.code.error meta.modelled phys.size.radius |
ADU |
Uncertainty in aperture-flux measurement, elliptical model based on the Kron radius |
wavg_flux_psf_g | double |
instr.det.psf instr.sensitivity |
ADU |
Weighted-average flux measurement of PSF fit single-epoch detections |
wavg_flux_psf_r | double |
instr.det.psf instr.sensitivity |
ADU |
Weighted-average flux measurement of PSF fit single-epoch detections |
wavg_flux_psf_i | double |
instr.det.psf instr.sensitivity |
ADU |
Weighted-average flux measurement of PSF fit single-epoch detections |
wavg_flux_psf_z | double |
instr.det.psf instr.sensitivity |
ADU |
Weighted-average flux measurement of PSF fit single-epoch detections |
wavg_flux_psf_y | double |
instr.det.psf instr.sensitivity |
ADU |
Weighted-average flux measurement of PSF fit single-epoch detections |
wavg_fluxerr_psf_g | double |
meta.code.error instr.det.psf instr.sensitivity |
ADU |
Uncertainty of weighted averaged flux measurement of PSF fit single-epoch detections |
wavg_fluxerr_psf_r | double |
meta.code.error instr.det.psf instr.sensitivity |
ADU |
Uncertainty of weighted averaged flux measurement of PSF fit single-epoch detections |
wavg_fluxerr_psf_i | double |
meta.code.error instr.det.psf instr.sensitivity |
ADU |
Uncertainty of weighted averaged flux measurement of PSF fit single-epoch detections |
wavg_fluxerr_psf_z | double |
meta.code.error instr.det.psf instr.sensitivity |
ADU |
Uncertainty of weighted averaged flux measurement of PSF fit single-epoch detections |
wavg_fluxerr_psf_y | double |
meta.code.error instr.det.psf instr.sensitivity |
ADU |
Uncertainty of weighted averaged flux measurement of PSF fit single-epoch detections |
class_star_g | double | scr.class |
Simple morphological extended source classifier. Values between 0 (galaxies) and 1 (stars). SPREAD_MODEL exhibits better performance for morphological classification. |
|
class_star_r | double | scr.class |
Simple morphological extended source classifier. Values between 0 (galaxies) and 1 (stars). SPREAD_MODEL exhibits better performance for morphological classification. |
|
class_star_i | double | scr.class |
Simple morphological extended source classifier. Values between 0 (galaxies) and 1 (stars). SPREAD_MODEL exhibits better performance for morphological classification. |
|
class_star_z | double | scr.class |
Simple morphological extended source classifier. Values between 0 (galaxies) and 1 (stars). SPREAD_MODEL exhibits better performance for morphological classification. |
|
class_star_y | double | scr.class |
Simple morphological extended source classifier. Values between 0 (galaxies) and 1 (stars). SPREAD_MODEL exhibits better performance for morphological classification. |
|
spread_model_g | double | scr.class |
Morphology based classifier based on comparison between a PSF versus exponential-PSF model. Values closer to 0 correspond to stars, larger values correspond to galaxies |
|
spread_model_r | double | scr.class |
Morphology based classifier based on comparison between a PSF versus exponential-PSF model. Values closer to 0 correspond to stars, larger values correspond to galaxies |
|
spread_model_i | double | scr.class |
Morphology based classifier based on comparison between a PSF versus exponential-PSF model. Values closer to 0 correspond to stars, larger values correspond to galaxies |
|
spread_model_z | double | scr.class |
Morphology based classifier based on comparison between a PSF versus exponential-PSF model. Values closer to 0 correspond to stars, larger values correspond to galaxies |
|
spread_model_y | double | scr.class |
Morphology based classifier based on comparison between a PSF versus exponential-PSF model. Values closer to 0 correspond to stars, larger values correspond to galaxies |
|
wavg_spread_model_g | double |
instr.sensitivity meta.modelled stat.value |
SPREAD MODEL using the weighted averaged values from single-epoch detections |
|
wavg_spread_model_r | double |
instr.sensitivity meta.modelled stat.value |
SPREAD MODEL using the weighted averaged values from single-epoch detections |
|
wavg_spread_model_i | double |
instr.sensitivity meta.modelled stat.value |
SPREAD MODEL using the weighted averaged values from single-epoch detections |
|
wavg_spread_model_z | double |
instr.sensitivity meta.modelled stat.value |
SPREAD MODEL using the weighted averaged values from single-epoch detections |
|
wavg_spread_model_y | double |
instr.sensitivity meta.modelled stat.value |
SPREAD MODEL using the weighted averaged values from single-epoch detections |
|
spreaderr_model_g | double |
meta.code.error instr.det.psf meta.modelled |
Uncertainty in morphology based classifier based on comparison between PSF versus exponential-PSF model. |
|
spreaderr_model_r | double |
meta.code.error instr.det.psf meta.modelled |
Uncertainty in morphology based classifier based on comparison between PSF versus exponential-PSF model. |
|
spreaderr_model_i | double |
meta.code.error instr.det.psf meta.modelled |
Uncertainty in morphology based classifier based on comparison between PSF versus exponential-PSF model. |
|
spreaderr_model_z | double |
meta.code.error instr.det.psf meta.modelled |
Uncertainty in morphology based classifier based on comparison between PSF versus exponential-PSF model. |
|
spreaderr_model_y | double |
meta.code.error instr.det.psf meta.modelled |
Uncertainty in morphology based classifier based on comparison between PSF versus exponential-PSF model. |
|
wavg_spreaderr_model_g | double |
meta.modelled instr.sensitivity |
Uncertainty in SPREAD MODEL using the weighted averaged values from single-epoch detections |
|
wavg_spreaderr_model_r | double |
meta.modelled instr.sensitivity |
Uncertainty in SPREAD MODEL using the weighted averaged values from single-epoch detections |
|
wavg_spreaderr_model_i | double |
meta.modelled instr.sensitivity |
Uncertainty in SPREAD MODEL using the weighted averaged values from single-epoch detections |
|
wavg_spreaderr_model_z | double |
meta.modelled instr.sensitivity |
Uncertainty in SPREAD MODEL using the weighted averaged values from single-epoch detections |
|
wavg_spreaderr_model_y | double |
meta.modelled instr.sensitivity |
Uncertainty in SPREAD MODEL using the weighted averaged values from single-epoch detections |