Hermes: Cosmic infrared background anisotropies and the clustering of dusty star-forming galaxies

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dc.contributor.authorViero, M. P.
dc.contributor.authorWang, L.
dc.contributor.authorZemcov, M.
dc.contributor.authorAddison, G.
dc.contributor.authorAmblard, A.
dc.contributor.authorArumugam, V.
dc.contributor.authorAussel, H.
dc.contributor.authorBethermin, M.
dc.contributor.authorBock, J.
dc.contributor.authorBoselli, A.
dc.contributor.authorBuat, V.
dc.contributor.authorBurgarella, D.
dc.contributor.authorCasey, C.M.
dc.contributor.authorClements, D.L.
dc.contributor.authorConley, A.
dc.contributor.authorConversi, L.
dc.contributor.authorCooray, Asantha
dc.contributor.authorde Zotti, G.
dc.contributor.authorDowell, C.D.
dc.contributor.authorFarrah, D.
dc.contributor.authorFranceschini, Alberto
dc.contributor.authorGlenn, J.
dc.contributor.authorGriffin, M.
dc.contributor.authorHatziminaoglou, Evanthia
dc.contributor.authorHeinis, S.
dc.contributor.authorIbar, Edo
dc.contributor.authorIvison, R.J.
dc.contributor.authorLagache, G.
dc.contributor.authorLevenson, L.
dc.contributor.authorMarchetti, L.
dc.contributor.authorMarsden, G.
dc.contributor.authorNguyen, H.T.
dc.contributor.authorOHalloran, B.
dc.contributor.authorOliver, S.J.
dc.contributor.authorOmont, A.
dc.contributor.authorPage, Matthew J.
dc.contributor.authorPapageorgiou, A.
dc.contributor.authorPearson, C.P.
dc.contributor.authorPerez-Fournon, I.
dc.contributor.authorPohlen, M.
dc.contributor.authorRigopoulou, D.
dc.contributor.authorRoseboom, I.G.
dc.contributor.authorRowan-Robinson, M.
dc.contributor.authorSchulz, B.
dc.contributor.authorScott, Douglas
dc.contributor.authorSeymour, N.
dc.contributor.authorShupe, D.L.
dc.contributor.authorSmith, A.J.
dc.contributor.authorSymeonidis, Myrto
dc.contributor.authorVaccari, M.
dc.contributor.authorValtchanov, I.
dc.contributor.authorVieira, J.D.
dc.contributor.authorWardlow, Julie L.
dc.contributor.authorXu, C.K.
dc.date.accessioned2016-01-12T09:41:53Z
dc.date.available2016-01-12T09:41:53Z
dc.date.issued2013
dc.description.abstractStar formation is well traced by dust, which absorbs the UV/optical light produced by young stars in actively starforming regions and re-emits the energy in the far-infrared/ submillimeter (FIR/submm; e.g., Savage & Mathis 1979). Roughly half of all starlight ever produced has been reprocessed by dusty star-forming galaxies (DSFGs; e.g., Hauser & Dwek 2001; Dole et al. 2006), and this emission is responsible for the ubiquitous cosmic infrared background (CIB; Puget et al. 1996; Fixsen et al. 1998). The mechanisms responsible for the presence or absence of star formation are partially dependent on the local environment (e.g., major mergers: Narayanan et al. 2010; condensation or cold accretion: Dekel et al. 2009, photoionization heating, supernovae, active galactic nuclei, and virial shocks: Birnboim & Dekel 2003; Granato et al. 2004; Bower et al. 2006). Thus, the specifics of the galaxy distribution—which can be determined statistically to high precision by measuring their clustering properties—inform the relationship of star formation and dark matter density, and are valuable inputs for models of galaxy formation. However, measuring the clustering of DSFGs has historically proven difficult to do.en_US
dc.description.accreditationWeb of Scienceen_US
dc.identifier.citationViero, M.P., et al., (2013). Hermes: Cosmic infrared background anisotropies and the clustering of dusty star-forming galaxies. The Astrophysical Journal , 772: 77en_US
dc.identifier.issn0004-637x
dc.identifier.urihttp://hdl.handle.net/10566/2054
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/772/1/77
dc.status.ispeerreviewedtrue
dc.subjectCosmic Infrared Background (CIB)en_US
dc.subjectGalaxiesen_US
dc.subjectHerschel Space Observatoryen_US
dc.subjectCosmologyen_US
dc.subjectStar formationen_US
dc.subjectGalaxy distributionen_US
dc.subjectDark matter densityen_US
dc.titleHermes: Cosmic infrared background anisotropies and the clustering of dusty star-forming galaxiesen_US
dc.typeArticleen_US

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