J/MNRAS/421/3027ivo://CDS.VizieR/J/MNRAS/421/3027doi:10.26093/cds/vizier.74213027CDSBourne N.Maddox S.J.Dunne L.Auld R.Baes M.Baldry I.K.,Bonfield D.G.Cooray A.Croom S.M.Dariush A.De Zotti G.Driver S.P.,Dye S.Eales S.Gomez H.L.Gonzalez-Nuevo J.Hopkins A.M.Ibar E.,Jarvis M.J.Lapi A.Madore B.Michalowski M.J.Pohlen M.Popescu C.C.,Rigby E.E.Seibert M.Smith D.J.B.Tuffs R.J.Van Der Werf P.,Brough S.Buttiglione S.Cava A.Clements D.L.Conselice C.J.,Fritz J.Hopwood R.Ivison R.J.Jones D.H.Kelvin L.S.Liske J.,Loveday J.Norberg P.Robotham A.S.G.Rodighiero G.Temi P.2024-07-17T20:15:20Z2013-04-12T15:10:04ZCDS support team

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

cds-question@unistra.frgalaxiesphotometrymillimeter-astronomysubmillimeter-astronomyWe use the Herschel-ATLAS survey to conduct the first large-scale statistical study of the submillimetre properties of optically selected galaxies. Using ~80000 r-band selected galaxies from 126deg^2^ of the GAMA survey, we stack into submillimetre imaging at 250, 350 and 500um to gain unprecedented statistics on the dust emission from galaxies at z<0.35. We find that low-redshift galaxies account for 5 per cent of the cosmic 250-um background (4 per cent at 350um; 3 per cent at 500um), of which approximately 60 per cent comes from 'blue' and 20 per cent from 'red' galaxies (rest-frame g-r).2012MNRAS.421.3027Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/421/3027CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/MNRAS/413/971 : Galaxy And Mass Assembly (GAMA) DR1 (Driver+, 2011)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/421/3027https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/421/3027http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/421/3027https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/421/3027https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/421/3027http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/421/3027GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tap3.972892068905477e-22 7.945784137810954e-22MillimeterdefaultJ/MNRAS/421/3027/table1Results of stacking in bins of g-r colour, redshift, and absolute magnituderecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintC[BGR] Colour bin Blue / Green / Redsrc.class.colorcharzMedian redshift in bin (2)src.redshiftfloatrMAGMedian absolute r magnitudemagphys.magAbsfloatNCount in the binphot.countintS250background-subtracted flux for SPIRE 250um bandmJyphot.flux.density;em.mm.750-1500GHzfloate_S250Statistical error on the median flux S250 (4)mJystat.errorfloatS/N250signal-to-noise ratio for SPIRE 250um bandstat.snrfloats250Measurement error (3)mJystat.errorfloatKS250KS probability that the distribution of fluxes in each bin is the same as that at a set of random positions, for SPIRE 250um bandstat.fit.goodnessfloatS350background-subtracted flux for SPIRE 350um bandmJyphot.flux.density;em.mm.750-1500GHzfloate_S350Statistical error on the median flux S350 (4)mJystat.errorfloatS/N350signal-to-noise ratio for SPIRE 350um bandstat.snrfloats350Measurement error (3)mJystat.errorfloatKS350KS probability that the distribution of fluxes in each bin is the same as that at a set of random positions, for SPIRE 350um bandstat.fit.goodnessfloatS500background-subtracted flux for SPIRE 500um bandmJyphot.flux.density;em.mm.400-750GHzfloate_S500Statistical error on the median flux S500 (4)mJystat.errorfloatS/N500signal-to-noise ratio for SPIRE 500um bandstat.snrfloats500Measurement error (3)mJystat.errorfloatKS500KS probability that the distribution of fluxes in each bin is the same as that at a set of random positions, for SPIRE 500um bandstat.fit.goodnessfloatK'250Median k-correction for SPIRE 250um band (5)magarith.factor;phot.magfloatK'350Median k-correction for SPIRE 350um band (5)magarith.factor;phot.magfloatK'500Median k-correction for SPIRE 500um band (5)magarith.factor;phot.magfloat