HerMES: The far-infrared emission from dust-obscured galaxies

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dc.contributor.authorCalanog, J.A.
dc.contributor.authorWardlow, Julie L.
dc.contributor.authorFu, Hai
dc.contributor.authorCooray, Asantha
dc.contributor.authorAssef, R.J.
dc.contributor.authorBock, J.
dc.contributor.authorCasey, C.M.
dc.contributor.authorConley, A.
dc.contributor.authorFarrah, D.
dc.contributor.authorIbar, Edo
dc.contributor.authorKartaltepe, J.
dc.contributor.authorMagdis, G.
dc.contributor.authorMarchetti, L.
dc.contributor.authorOliver, S.J.
dc.contributor.authorPerez-Fournon, I.
dc.contributor.authorRiechers, D.
dc.contributor.authorRigopoulou, D.
dc.contributor.authorRoseboom, I.G.
dc.contributor.authorSchulz, B.
dc.contributor.authorScott, Douglas
dc.contributor.authorSymeonidis, Myrto
dc.contributor.authorVaccari, M.
dc.contributor.authorViero, M. P.
dc.contributor.authorZemcov, M.
dc.date.accessioned2016-01-13T08:55:22Z
dc.date.available2016-01-13T08:55:22Z
dc.date.issued2013
dc.description.abstractThe far-infrared (far-IR) luminosities of luminous infrared galaxies (LIRGs) and ultra-LIRGs (ULIRGs) are dominated by reprocessed thermal dust emission, due to a combination of star formation and active galactic nucleus (AGN) activity, with star formation typically being the more dominant component (e.g., Watabe et al. 2009; Elbaz et al. 2010). Locally, these sources are rare, although out to z - 1 they become more numerous and increasingly dominate the IR luminosity function of galaxies with increasing redshift (e.g., Le Floc’h et al. 2005; P´erez-Gonz´alez et al. 2005; Caputi et al. 2007; Magnelli et al. 2009; Rodighiero et al. 2010; Eales et al. 2010). (U)LIRGs are thought to trace a phase of intense star formation activity, which is likely followed by, or partially concurrent with, an episode of vigorous black hole accretion. It is postulated that upon the cessation of these phases, each produces an early-type galaxy (Genzel et al. 2001; Farrah et al. 2003; Lonsdale et al. 2006; Veilleux et al. 2009).en_US
dc.description.accreditationWeb of Scienceen_US
dc.identifier.citationCalanog, J., et al., (2013). HerMES: The far-infrared emission from dust-obscured galaxies. The Astrophysical Journal , 775(61)en_US
dc.identifier.issn0004-637x
dc.identifier.urihttp://hdl.handle.net/10566/2056
dc.language.isoenen_US
dc.privacy.showsubmitterfalse
dc.publisherAmerican Astronomical Societyen_US
dc.rightsAAS grants back to authors the non-exclusive right of republication, subject only to giving appropriate credit to the journal in which the article was published. This non-exclusive right of republication gives authors the right to approve or deny reproduction of all or part of the article and to post the final published version online.
dc.source.urihttp://dx.doi.org/10.1088/0004-637X/775/1/61
dc.status.ispeerreviewedtrue
dc.subjectCosmologyen_US
dc.subjectGalaxiesen_US
dc.subjectLuminosity functionen_US
dc.subjectStar formationen_US
dc.subjectLuminous infrared galaxies (LRGs)en_US
dc.subjectActive galactic nucleus (AGN)en_US
dc.subjectThermal dust emissionen_US
dc.titleHerMES: The far-infrared emission from dust-obscured galaxiesen_US
dc.typeArticleen_US

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