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dc.contributor.authorDariush, A.
dc.contributor.authorCortese, L.
dc.contributor.authorEales, S.
dc.contributor.authorPascale, E.
dc.contributor.authorSmith, M. W. L.
dc.contributor.authorDunne, L.
dc.contributor.authorDye, S.
dc.contributor.authorScott, D.
dc.contributor.authorAuld, R.
dc.contributor.authorBaes, M.
dc.contributor.authorBland-Hawthorn, J.
dc.contributor.authorButtiglione, S.
dc.contributor.authorCava, A.
dc.contributor.authorClements, D. L.
dc.contributor.authorCooray, A.
dc.contributor.authorDezotti, G.
dc.contributor.authorDriver, S.
dc.contributor.authorFritz, J.
dc.contributor.authorGomez, H.L.
dc.contributor.authorHopkins, A.
dc.contributor.authorHopwood, R.
dc.contributor.authorIvison, R.J.
dc.contributor.authorJarvis, M.J.
dc.contributor.authorJones, D. H.
dc.contributor.authorKelvin, L.
dc.contributor.authorKhosroshahi, H. G.
dc.contributor.authorLiske, J.
dc.contributor.authorLoveday, J.
dc.contributor.authorMaddox, S.
dc.contributor.authorMadore, B. F.
dc.contributor.authorMichalowski, M. J.
dc.contributor.authorNorberg, P.
dc.contributor.authorPhillipps, S.
dc.contributor.authorPohlen, M.
dc.contributor.authorPopescu, C. C.
dc.contributor.authorPrescott, M.
dc.contributor.authorRigby, E.
dc.contributor.authorRobotham, A.
dc.contributor.authorRodighiero, G.
dc.contributor.authorSeibert, M.
dc.contributor.authorSmith, Daniel
dc.contributor.authorTemi, P.
dc.contributor.authorTuffs, R. J.
dc.contributor.authorvan der Werf, P.
dc.date.accessioned2011-12-14T17:01:13Z
dc.date.available2011-12-14T17:01:13Z
dc.date.issued2011-11-01
dc.identifier.citationDariush , A , Cortese , L , Eales , S , Pascale , E , Smith , M W L , Dunne , L , Dye , S , Scott , D , Auld , R , Baes , M , Bland-Hawthorn , J , Buttiglione , S , Cava , A , Clements , D L , Cooray , A , Dezotti , G , Driver , S , Fritz , J , Gomez , H L , Hopkins , A , Hopwood , R , Ivison , R J , Jarvis , M J , Jones , D H , Kelvin , L , Khosroshahi , H G , Liske , J , Loveday , J , Maddox , S , Madore , B F , Michalowski , M J , Norberg , P , Phillipps , S , Pohlen , M , Popescu , C C , Prescott , M , Rigby , E , Robotham , A , Rodighiero , G , Seibert , M , Smith , D , Temi , P , Tuffs , R J & van der Werf , P 2011 , ' The environment and characteristics of low-redshift galaxies detected by the Herschel-ATLAS ' , Monthly Notices of the Royal Astronomical Society , vol. 418 , no. 1 , pp. 64-73 . https://doi.org/10.1111/j.1365-2966.2011.19340.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 496960
dc.identifier.otherPURE UUID: 96578bf7-220a-44ca-b3ac-bb998a087663
dc.identifier.otherBibtex: urn:45ed63a50c6ee1b71a5983ef5f009d3a
dc.identifier.otherScopus: 81055156608
dc.identifier.urihttp://hdl.handle.net/2299/7290
dc.description.abstractWe investigate the ultraviolet and optical properties and environment of low-redshift galaxies detected in the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) science demonstration data. We use the Sloan Digital Sky Survey seventh release and the Galaxy and Mass Assembly data base to select galaxies with mag in the redshift range 0.02=z=0.2 and look for their submillimetre counterparts in H-ATLAS. Our results show that at low redshift, H-ATLAS detects mainly blue/star-forming galaxies with a minor contribution from red systems which are highly obscured by dust. In addition we find that the colour of a galaxy rather than the local density of its environment determines whether it is detectable by H-ATLAS. The average dust temperature of galaxies that are simultaneously detected by both PACS and SPIRE is 25 +/- 4K, independent of environment. This analysis provides a glimpse of the potential of the H-ATLAS data to investigate the submillimetre properties of galaxies in the local universe.en
dc.format.extent10
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.rightsEmbargoed
dc.subjectmethods: data analysis, galaxies: general, galaxies: statistics, submillimetre: galaxies, submillimetre: general
dc.titleThe environment and characteristics of low-redshift galaxies detected by the Herschel-ATLASen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.date.embargoedUntil2012-05-01
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeFinal Accepted Version
dcterms.dateAccepted2011-11-01
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1111/j.1365-2966.2011.19340.x
rioxxterms.licenseref.startdate2012-05-01
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.date.embargo2012-05-01
herts.rights.accesstypeEmbargoed


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