J/ApJ/769/80ivo://CDS.VizieR/J/ApJ/769/80doi:10.26093/cds/vizier.17690080CDSAshby M.L.N.Willner S.P.Fazio G.G.Huang J.-S.Arendt R.Barmby P.,Barro G.Bell E.F.Bouwens R.Cattaneo A.Croton D.Dave R.,Dunlop J.S.Egami E.Faber S.Finlator K.Grogin N.A.Guhathakurta P.,Hernquist L.Hora J.L.Illingworth G.Kashlinsky A.Koekemoer A.M.,Koo D.C.Labbe I.Li Y.Lin L.Moseley H.Nandra K.Newman J.,Noeske K.Ouchi M.Peth M.Rigopoulou D.Robertson B.Sarajedini V.,Simard L.Smith H.A.Wang Z.Wechsler R.Weiner B.Wilson G.,Wuyts S.Yamada T.Yan H.2017-06-26T11:48:54Z2015-01-15T13:07:22ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frgalaxiesinfrared-sourcesinfrared-photometrysurveysThe Spitzer Extended Deep Survey (SEDS) is a very deep infrared survey within five well-known extragalactic science fields: the UKIDSS Ultra-Deep Survey, the Extended Chandra Deep Field South, COSMOS, the Hubble Deep Field North, and the Extended Groth Strip. SEDS covers a total area of 1.46deg^2^ to a depth of 26 AB mag (3{sigma}) in both of the warm Infrared Array Camera (IRAC) bands at 3.6 and 4.5{mu}m. Because of its uniform depth of coverage in so many widely-separated fields, SEDS is subject to roughly 25% smaller errors due to cosmic variance than a single-field survey of the same size. SEDS was designed to detect and characterize galaxies from intermediate to high redshifts (z=2-7) with a built-in means of assessing the impact of cosmic variance on the individual fields. Because the full SEDS depth was accumulated in at least three separate visits to each field, typically with six-month intervals between visits, SEDS also furnishes an opportunity to assess the infrared variability of faint objects. This paper describes the SEDS survey design, processing, and publicly-available data products. Deep IRAC counts for the more than 300000 galaxies detected by SEDS are consistent with models based on known galaxy populations. Discrete IRAC sources contribute 5.6+/-1.0 and 4.4+/-0.8nW/m2/sr at 3.6 and 4.5{mu}m to the diffuse cosmic infrared background (CIB). IRAC sources cannot contribute more than half of the total CIB flux estimated from DIRBE data. Barring an unexpected error in the DIRBE flux estimates, half the CIB flux must therefore come from a diffuse component.2013ApJ...769...80Ahttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/769/80CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toII/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012)II/284 : COSMOS Multi-Wavelength Photometry Catalog (Capak+, 2007)VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)II/261 : GOODS initial results (Giavalisco+, 2004)I/284 : The USNO-B1.0 Catalog (Monet+ 2003)J/A+A/544/A156 : UltraVISTA Catalogue Release DR1 (McCracken+, 2012)J/ApJ/727/1 : IRAC/MUSYC SIMPLE survey (Damen+, 2011)J/ApJS/193/30 : UV-to-FIR analysis of sources in the EGS. II. (Barro+, 2011)J/ApJS/193/13 : Spitzer/IRAC sources in the EGS I. SEDs (Barro+, 2011)J/ApJS/187/251 : Ultradeep Ks imaging in the GOODS-N (Wang+, 2010)J/ApJ/717/1181 : Spitzer power-law galaxies in EGS (Park+, 2010)J/ApJ/716/530 : Mid-IR variability from the SDWFS (Kozlowski+, 2010)J/ApJ/697/506 : Mid-infrared galaxy luminosity function from AGN (Dai+, 2009)J/ApJ/680/130 : Mid-IR colors of AGNs in the MUSYC ECDF-S (Cardamone+, 2008)J/ApJS/177/431 : Mid-IR sources in EGS (Barmby+, 2008)J/AJ/132/2159 : IRAC counterparts of 6cm galaxies in EGS (Willner+, 2006)J/ApJ/596/748 : IR Observations in HDF-North (Thompson+, 2003)J/AJ/112/1335 : Hubble Deep Field observations (Williams+ 1996)J/AJ/105/1860 : 2-35 micron point source IR sky model (Cohen, 1993)http://www.cfa.harvard.edu/SEDS : SEDS home pagehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/769/80https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/769/80http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/769/80https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/769/80https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/769/80http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/769/80GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/769/80/catalog (Spitzer Extended Deep Survey full-depth source catalog for the UDS, ECDFS, COSMOS, HDFN and EGS fields)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/769/80/catalog?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/769/80/catalog?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/769/80/catalog?GETtext/xml+votable180.050000true34.17434-5.277630.005555555555555556Cone search capability for table J/ApJ/769/80/table1 (The five Spitzer Extended Deep Survey (SEDS) fields)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/769/80/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/769/80/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/769/80/table1?GETtext/xml+votable180.050000true34.5-5.171390.0055555555555555566/11230 11249 11252 11424 11425 11428 17677 17679 17688 17690 27256 27258 27259 35935 359574.414320678087048e-20 5.517906024225661e-20https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/769/80?format=asciiInfrareddefaultJ/ApJ/769/80/catalogSpitzer Extended Deep Survey full-depth source catalog for the UDS, ECDFS, COSMOS, HDFN and EGS fieldsRAJ2000Right Ascension (J2000) at 3.6umdegpos.eq.ra;meta.mainindexedrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSEDSSEDS identifier; Jhhmmss.ss-ddmmss.smeta.id;meta.maincharindexedDEJ2000Declination (J2000) at 3.6umdegpos.eq.dec;meta.mainindexed[3.6]psf[13.9/26.6] PSF-fitted 3.6um band AB magnitudemagphot.mag;em.IR.3-4umfloat[3.6]2.4?=0 The 3.6um band mag; 2.4" aperture (1)magphot.mag;em.IR.3-4umfloatnullablee_[3.6]2.4The 1{sigma} uncertainty in A2.4-3.6magmagstat.errorfloat[3.6]3.6?=0 The 3.6um band mag; 3.6" aperture (1)magphot.mag;em.IR.3-4umfloatnullable[3.6]4.8?=0 The 3.6um band mag; 4.8" aperture (1)magphot.mag;em.IR.3-4umfloatnullable[3.6]6.0[13/39]?=0 The 3.6um band magnitude; 6.0" aperture (1)magphot.mag;em.IR.3-4umfloatnullable[3.6]7.2?=0 The 3.6um band mag; 7.2" aperture (1)magphot.mag;em.IR.3-4umfloatnullable[3.6]12?=0 The 3.6um band magnitude; 12" aperture (1)magphot.mag;em.IR.3-4umfloatnullableC3.6Effective 3.6 um coverage (2)meta.numberintf3.6? Sum of flags for 3.6 um photometry (3)meta.codeintnullable[4.5]psfPSF-fitted 4.5 um band AB magnitudemagphot.mag;em.IR.4-8umfloat[4.5]2.4?=0 The 4.5um band mag; 2.4" aperture (1)magphot.mag;em.IR.4-8umfloatnullablee_[4.5]2.4The 1{sigma} uncertainty in A2.4-4.5magmagstat.errorfloat[4.5]3.6?=0 The 4.5um band mag; 3.6" aperture (1)magphot.mag;em.IR.4-8umfloatnullable[4.5]4.8?=0 The 4.5um band mag; 4.8" aperture (1)magphot.mag;em.IR.4-8umfloatnullable[4.5]6.0[13/38]?=0 The 4.5um band mag; 6.0" aperture (1)magphot.mag;em.IR.4-8umfloatnullable[4.5]7.2?=0 The 4.5um band mag; 7.2" aperture (1)magphot.mag;em.IR.4-8umfloatnullable[4.5]12?=0 The 4.5um band magnitude; 12" aperture (1)magphot.mag;em.IR.4-8umfloatnullableC4.5Effective 4.5 um coverage (2)meta.numberintf4.5? Sum of flags for 4.5 um photometry (3)meta.codeintnullableTblSimbad column added by the CDSmeta.id;meta.datasetintnullableJ/ApJ/769/80/table1The five Spitzer Extended Deep Survey (SEDS) fieldsFieldField nameobs.fieldcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTblTable number of the catalog containing the fieldmeta.id;meta.datasetintnullableRAJ2000Hour of right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Degree of declination (J2000)pos.eq.dec;meta.mainArea[0.19/0.35] Field area (1)deg**2phys.angSizefloatPID[8/70204] Spitzer program ID numbermeta.id;obsintDate1First date of observationtime.epoch;obsnullableDate2Other date of observationtime.epoch;obsnullableBCD3.6um, 4.5um Basic Calibrated Data usedinstr.calibcharn_BCD[bc] Flag on BCD: b=30s frames; c=200s framesmeta.notechar