J/MNRAS/456/2221ivo://CDS.VizieR/J/MNRAS/456/2221doi:10.26093/cds/vizier.74562221CDSDariush A.Dib S.Hony S.Smith D.J.B.Zhukovska S.Dunne L.,Eales S.Andrae E.Baes M.Baldry I.Bauer A.Bland-Hawthorn J.,Brough S.Bourne N.Cava A.Clements D.Cluver M.Cooray A.,De Zotti G.Driver S.Grootes M.W.Hopkins A.M.Hopwood R.Kaviraj S.,Kelvin L.Lara-Lopez M.A.Liske J.Loveday J.Maddox S.Madore B.,Michalowski M.J.Pearson C.Popescu C.Robotham A.Rowlands K.,Seibert M.Shabani F.Smith M.W.L.Taylor E.N.Tuffs R.Valiante E.,Virdee J.S.2024-08-15T20:17:22Z2016-11-16T09:08:01ZCDS support team

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

cds-question@unistra.frgalaxiesphotometrygalaxy-classification-systemsWe combine Herschel/SPIRE submillimetre (submm) observations with existing multiwavelength data to investigate the characteristics of low-redshift, optically red galaxies detected in submm bands. We select a sample of galaxies in the redshift range 0.01<=z<=0.2, having >5{sigma} detections in the SPIRE 250{mu}m submm waveband. Sources are then divided into two sub-samples of red and blue galaxies, based on their UV-optical colours. Galaxies in the red sample account for ~4.2 per cent of the total number of sources with stellar masses M*>~10^10^M_{sun}_. Following visual classification of the red galaxies, we find that >~30 per cent of them are early-type galaxies and >~40 per cent are spirals. The colour of the red-spiral galaxies could be the result of their highly inclined orientation and/or a strong contribution of the old stellar population. It is found that irrespective of their morphological types, red and blue sources occupy environments with more or less similar densities (i.e. the {Sigma}_5_ parameter). From the analysis of the spectral energy distributions of galaxies in our samples based on MAGPHYS, we find that galaxies in the red sample (of any morphological type) have dust masses similar to those in the blue sample (i.e. normal spiral/star-forming systems). However, in comparison to the red-spirals and in particular blue systems, red-ellipticals have lower mean dust-to-stellar mass ratios. Besides galaxies in the red-elliptical sample have much lower mean star formation/specific star formation rates in contrast to their counterparts in the blue sample. Our results support a scenario where dust in early-type systems is likely to be of an external origin.2016MNRAS.456.2221Dhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/456/2221CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/MNRAS/415/2336 : Herschel-ATLAS Science Demonstration Catalog (Rigby+, 2011)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/456/2221https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/456/2221http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/456/2221https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/456/2221https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/456/2221http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/456/2221GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/456/2221/tablea1 (List of all red galaxies detected in HATLAS)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/456/2221/tablea1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/456/2221/tablea1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/456/2221/tablea1?GETtext/xml+votable180.050000true133.709252.2023250.005555555555555556Cone search capability for table J/MNRAS/456/2221/tablea2 (MAGPHYS output parameters for the red galaxies having WISE observed photometric data)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/456/2221/tablea2?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/456/2221/tablea2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/456/2221/tablea2?GETtext/xml+votable180.050000true177.349167-1.0836110.0055555555555555565/6399 6570 6740-6741 6825 6/4098 4101 4104 21843-21845 21847-21849 21851 21854-21855 21873-21874 21876-21877 25919 25931 25935 25938 25942 25947 25949 25951-25952 25954-25955 25958-25960 25962-25963 25965 25967-25968 26004 26050-26051 26254 26274-26277 26279 26956-26957 26968-26969 26972-26973 26993 27279 27290 27299 27305 27310-27311 27313 27321 27324 27648-27649 40958https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/456/2221?format=asciiOpticaldefaultJ/MNRAS/456/2221/tablea1List of all red galaxies detected in HATLASobjIdSDSS objIdmeta.idrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIndex[1/117] Indexmeta.idintMAGPHYSindicates MAGPHYS output parameters in tablea2meta.ref.urlcharHATLASHATLAS IAU name (JHHMMSS.s+DDMMSS)meta.id;meta.maincharprimaryRAJ2000SDSS right ascension (J2000)pos.eq.ra;meta.mainDEJ2000SDSS declination (J2000)pos.eq.dec;meta.mainNUV-rNUV-r colour indexmagphot.color;em.UV;em.optfloatlog({Sigma}5)? Surface density to the fifth nearest neighbourlog(Mpc**-2)src.densityfloatnullableiInclinationdegsrc.orbital.inclinationfloatType[USE] Type (1)src.classcharSloanDisplay the online SDSS data for this galaxymeta.ref.urlcharSimbadSimbad column added by the CDSmeta.ref.urlcharJ/MNRAS/456/2221/tablea2MAGPHYS output parameters for the red galaxies having WISE observed photometric datarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIndex[1/78] Indexmeta.idintHATLASHATLAS IAU name (JHHMMSS.s+DDMMSS)meta.id;meta.maincharlogM*Stellar masslog(solMass)phys.massfloatlog(SFR)Star formation ratelog(solMass.yr**-1)phys.SFRfloatlog(SFR/M*)Spectific star formation ratelog(yr**-1)phys.SFRfloatlog(MD)Dust masslog(solMass)phys.massfloatlog(MD/M*)Dust to stellar mass ratiophys.mass;arith.ratiofloatfmuFraction of total dust luminosity contributed by the diffuse interstellar medium (1)phys.luminosity;arith.ratiofloatWISEDisplay the WISE (Cutri et al., 2012, Cat. II/311) data witihn 5"meta.ref.urlchar_RAPositinos from HATLAS name (right ascension part)degpos.eq.ra;meta.main_DEPositinos from HATLAS name (declination part)degpos.eq.dec;meta.main