J/ApJ/769/116ivo://CDS.VizieR/J/ApJ/769/116doi:10.26093/cds/vizier.17690116CDSHwang H.S.Geller M.J.2017-07-03T14:25:37Z2014-06-23T12:25:27ZCDS support team

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

cds-question@unistra.frinfrared-photometryultraviolet-photometryvisible-astronomysloan-photometrygalaxiesinfrared-sourcesredshiftedsurveysWe use Wide-field Infrared Survey Explorer (WISE), AKARI, and Galaxy Evolution Explorer (GALEX) data to select local analogs of high-redshift (z~2) dust obscured galaxies (DOGs). We identify 47 local DOGs with S_12{mu}m_/S_0.22{mu}m_>=892 and S_12{mu}m_>20mJy at 0.05<z<0.08 in the Sloan Digital Sky Survey data release 7. The infrared (IR) luminosities of these DOGs are in the range 3.4x10^10^(L_{sun}_)<~L_IR_<~7.0x10^11^(L_{sun}_) with a median L_IR_ of 2.1x10^11^(L_{sun}_). We compare the physical properties of local DOGs with a control sample of galaxies that have lower S_12{mu}m_/S_0.22{mu}m_ but have similar redshift, IR luminosity, and stellar mass distributions. Both WISE 12{mu}m and GALEX near-ultraviolet (NUV) flux densities of DOGs differ from the control sample of galaxies, but the difference is much larger in the NUV. Among the 47 DOGs, 36%+/-7% have small axis ratios in the optical (i.e., b/a<0.6), larger than the fraction among the control sample (17%+/-3%). There is no obvious sign of interaction for many local DOGs. No local DOGs have companions with comparable optical magnitudes closer than ~50kpc. The large- and small-scale environments of DOGs are similar to the control sample. Many physical properties of local DOGs are similar to those of high-z DOGs, even though the IR luminosities of local objects are an order of magnitude lower than for the high-z objects: the presence of two classes (active galactic nuclei- and star formation-dominated) of DOGs, abnormal faintness in the UV rather than extreme brightness in the mid-IR, and diverse optical morphology. These results suggest a common underlying physical origin of local and high-z DOGs. Both seem to represent the high-end tail of the dust obscuration distribution resulting from various physical mechanisms rather than a unique phase of galaxy evolution.2013ApJ...769..116Hhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/769/116CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toV/139 : The SDSS Photometric Catalog, Release 9 (Adelman-McCarthy+, 2012)II/311 : WISE All-Sky Data Release (Cutri+ 2012)II/298 : AKARI/FIS All-Sky Survey Point Source Catalogues (ISAS/JAXA, 2010)II/297 : AKARI/IRC mid-IR all-sky Survey (ISAS/JAXA, 2010)II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009)VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)II/156 : IRAS Faint Source Catalog, |b| > 10, Version 2.0 (Moshir+ 1989)J/ApJ/744/150 : Dust-obscured galaxies (DOGs) at z=~2 (Bussmann+, 2012)J/AJ/143/125 : SED of 113 dust-obscured galaxies at z~2 (Melbourne+, 2012)J/A+A/533/A119 : GOODS-Herschel North and South catalogs (Elbaz+, 2011)J/ApJS/182/628 : Spitzer quasar and ULIRG evolution study (Veilleux+, 2009)J/ApJ/692/422 : MAMBO observations of SWIRE sources (Lonsdale+, 2009)J/ApJ/663/81 : SED of hard X-ray selected AGN in XMDS (Polletta+, 2007)J/ApJS/173/293 : UV-Optical galaxy color-magnitude diagram I. (Wyder+, 2007)J/PASP/117/227 : Properties of 101 galaxies from the NFGS (Kewley+, 2005)J/ApJ/622/772 : Redshift survey of submillimeter galaxies (Chapman+, 2005)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/769/116https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/769/116http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/769/116https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/769/116https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/769/116http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/769/116GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/769/116/dogs (Properties and UV to FIR photometry for WISE 12um selected dust-obscured galaxies (DOGs))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/769/116/dogs?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/769/116/dogs?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/769/116/dogs?GETtext/xml+votable180.050000true3.1117917-0.80540280.0055555555555555566/4097 5239 5249 5296 5329 5702 5962 6009 6477 6544 6915 7209 7502 7566 8248 8693 8695 8997 9328 9660 10099 10270 10281 10305 10321 10339 10591 10771 11006 18083 18831 25531 26220 27078 27307 27393 27433 27559 27631 27871 27976 28113 28494 31387 31530 32441 367821.1655134642791134e-21 1.4134638842407062e-18https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/769/116?format=asciiUVOpticalInfrareddefaultJ/ApJ/769/116/dogsProperties and UV to FIR photometry for WISE 12um selected dust-obscured galaxies (DOGs)SDSSSDSS-DR9 name (JHHMMSS.ss+DDMMSS.s)meta.id;meta.maincharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/47] Running sequence numbermeta.idintprimaryobjIDSDSS-DR9 ObjIDmeta.idRAJ2000Hour of right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Degree of declination (J2000)pos.eq.dec;meta.mainz[0.05/0.08] Redshiftsrc.redshiftfloatM*[1.56/41.95]? Stellar mass (1)1e+10solMassphys.massfloatnullablee_M*[0.34/10.45]? M* uncertainty (1)1e+10solMassstat.errorfloatnullablel_LirLimit flag on Lirmeta.code.errorcharLir[3.42/68.74] IR luminosity1e+10solLumphys.luminosity;em.IRfloate_Lir[0.09/5.9]? Lir uncertainty1e+10solLumstat.errorfloatnullablel_fAGNLimit flag on fAGNmeta.code.errorcharfAGN[0/100] AGN contribution to the total IR luminosity%phys.luminosity;arith.ratiointe_fAGN[0/10]? fAGN uncertainty%stat.errorintnullableClClassification (2)meta.code.classchar2MXCross-match with 2MASX (Cat. VII/233) within 3"meta.ref.urlintnullableAKACross-match with AKARI (Cat. II/297 and II/298) within 5"meta.ref.urlintnullableIRSCross-match with IRAS FSC (Cat. II/156) within 10"meta.ref.urlintnullableWISEDisplay the WISE data (Cat. II/311) within 3"meta.ref.urlcharSEDSimbad column added by the CDSmeta.ref.urlcharSloanDisplay the SDSS data for this galaxymeta.ref.urlcharSimbadSimbad column added by the CDSmeta.ref.urlcharNEDSimbad column added by the CDSmeta.refcharFUV[19.5/22.7]? GALEX FUV magnitude (3)magphot.mag;em.UV.100-200nmfloatnullablee_FUV[0.05/0.5]? FUV uncertainty (3)magstat.errorfloatnullableNUV[18.3/22.8] GALEX NUV magnitude (3)magphot.mag;em.UVfloate_NUV[0.04/0.7] NUV uncertainty (3)magstat.errorfloatumag[16.6/20.5] SDSS Petrosian u-band magnitude (3)magphot.mag;em.opt.Ufloate_umag[0.02/0.7] umag uncertainty (3)magstat.error;phot.mag;em.opt.Ufloatgmag[15.3/18.4] SDSS Petrosian g-band magnitude (3)magphot.mag;em.opt.Bfloate_gmag[0/0.4] gmag uncertainty (3)magstat.error;phot.mag;em.opt.Bfloatrmag[14.6/17.6] SDSS Petrosian r-band magnitude (3)magphot.mag;em.opt.Rfloate_rmag[0/0.4] rmag uncertainty (3)magstat.error;phot.mag;em.opt.Rfloatimag[14.3/17.2] SDSS Petrosian i-band magnitude (3)magphot.mag;em.opt.Ifloate_imag[0/0.4] imag uncertainty (3)magstat.error;phot.mag;em.opt.Ifloatzmag[14.1/17] SDSS Petrosian z-band magnitude (3)magphot.mag;em.opt.Ifloate_zmag[0.01/0.3] zmag uncertainty (3)magstat.error;phot.mag;em.opt.IfloatJmag[13.7/16.3]? 2MASS J-band magnitude (4)magphot.mag;em.IR.Jfloatnullablee_Jmag[0.03/0.2]? Jmag uncertaintymagstat.error;phot.mag;em.IR.JfloatnullableHmag[13.3/16]? 2MASS H-band magnitude (4)magphot.mag;em.IR.Hfloatnullablee_Hmag[0.03/0.2]? Hmag uncertaintymagstat.error;phot.mag;em.IR.HfloatnullableKsmag[13/16]? 2MASS Ks-band magnitude (4)magphot.mag;em.IR.Kfloatnullablee_Ksmag[0.03/0.2]? Ksmag uncertaintymagstat.error;phot.mag;em.IR.KfloatnullableS3.4[0.7/36.5] WISE 3.4um flux densitymJyphot.mag;em.IR.3-4umfloate_S3.4[0.02/0.8] S3.4 uncertaintymJystat.errorfloatS4.6[1/55.5] WISE 4.6 flux densitymJyphot.mag;em.IR.4-8umfloate_S4.6[0.03/1] S4.6 uncertaintymJystat.errorfloatS9[65/138.2]? AKARI/IRC 9um flux densitymJyphot.flux.density;em.IR.8-15umfloatnullablee_S9[2.4/25]? S9 uncertaintymJystat.errorfloatnullableS12[21.7/160.3] WISE 12um flux densitymJyphot.flux.density;em.IR.8-15umfloate_S12[0.3/2.3] S12 uncertaintymJystat.errorfloatS12i[81.6/162.8]? IRAS FSC 12um flux densitymJyphot.flux.density;em.IR.8-15umfloatnullablee_S12i[14.9/30.7]? S12i uncertaintymJystat.errorfloatnullableS18[94/344]? AKARI/IRC 18um flux densitymJyphot.flux.density;em.IR.8-15umfloatnullablee_S18[8/51]? S18 uncertaintymJystat.errorfloatnullableS22[34/619] WISE 22um flux densitymJyphot.flux.density;em.IR.15-30umfloate_S22[1/11] S22 uncertaintymJystat.errorfloatS25[127/717]? IRAS FSC 25um flux densitymJyphot.flux.density;em.IR.15-30umfloatnullablee_S25[15/58]? S25 uncertaintymJystat.errorfloatnullableS60[0.2/5.2]? IRAS FSC 60um flux densityJyphot.flux.density;em.IR.30-60umfloatnullablee_S60[0.04/0.4]? S60 uncertaintyJystat.errorfloatnullableS65[2.9/3.8]? AKARI/FIS 65um flux densityJyphot.flux.density;em.IR.30-60umfloatnullablee_S65[0.2/0.5]? S65 uncertaintyJystat.errorfloatnullableS90[0.5/5.1]? AKARI/FIS 90um flux densityJyphot.flux.density;em.IR.60-100umfloatnullablee_S90[0.02/0.3]? S90 uncertaintyJystat.errorfloatnullableS100[0.5/5.1]? IRAS FSC 100um flux densityJyphot.flux.density;em.IR.60-100umfloatnullablee_S100[0.1/0.6]? S100 uncertaintyJystat.errorfloatnullableS140[2.8/6]? AKARI/FIS 140um flux densityJyphot.flux.density;em.mm.1500-3000GHzfloatnullablee_S140[0.3/1.3]? S140 uncertaintyJystat.errorfloatnullable