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dc.contributor.authorCooray, A.
dc.contributor.authorAmblard, A.
dc.contributor.authorArumugam, V.
dc.contributor.authorWang, L.
dc.contributor.authorAuld, R.
dc.contributor.authorAussel, H.
dc.contributor.authorBabbedge, T.
dc.contributor.authorBlain, A.
dc.contributor.authorBock, J.
dc.contributor.authorBoselli, A.
dc.contributor.authorBuat, V.
dc.contributor.authorBurgarella, D.
dc.contributor.authorCastro-Rodriguez, N.
dc.contributor.authorCava, A.
dc.contributor.authorChanial, P.
dc.contributor.authorClements, D. L.
dc.contributor.authorConley, A.
dc.contributor.authorConversi, L.
dc.contributor.authorDowell, C.D.
dc.contributor.authorDwek, E.
dc.contributor.authorEales, S.
dc.contributor.authorElbaz, D.
dc.contributor.authorFarrah, D.
dc.contributor.authorFox, M.
dc.contributor.authorFranceschini, A.
dc.contributor.authorGear, W.
dc.contributor.authorGlenn, J.
dc.contributor.authorGriffin, M.
dc.contributor.authorHalpern, M.
dc.contributor.authorHatziminaoglou, E.
dc.contributor.authorIbar, E.
dc.contributor.authorIsaak, K.
dc.contributor.authorIvison, R.J.
dc.contributor.authorKhostovan, A.A.
dc.contributor.authorLagache, G.
dc.contributor.authorLevenson, L.
dc.contributor.authorLu, N.
dc.contributor.authorMadden, S.
dc.contributor.authorMaffei, B.
dc.contributor.authorMainetti, G.
dc.contributor.authorMarchetti, L.
dc.contributor.authorMarsden, G.
dc.contributor.authorMitchell-Wynne, K.
dc.contributor.authorMortier, A. M. J.
dc.contributor.authorNguyen, H.T.
dc.contributor.authorO'Halloran, B.
dc.contributor.authorOliver, S. J.
dc.contributor.authorOmont, A.
dc.contributor.authorPage, M.J.
dc.contributor.authorPanuzzo, P.
dc.contributor.authorPapageorgiou, A.
dc.contributor.authorPearson, C.P.
dc.contributor.authorPerez Fournon, I.
dc.contributor.authorPohlen, M.
dc.contributor.authorRawlings, J.I.
dc.contributor.authorRaymond, G.
dc.contributor.authorRigopoulou, D.
dc.contributor.authorRizzo, D.
dc.contributor.authorRoseboom, I.G.
dc.contributor.authorRowan-Robinson, M.
dc.contributor.authorSchulz, B.
dc.contributor.authorScott, D.
dc.contributor.authorSerra, P.
dc.contributor.authorSeymour, N.
dc.contributor.authorShupe, D. L.
dc.contributor.authorSmith, A. J.
dc.contributor.authorStevens, Jason
dc.contributor.authorSymeonidis, M.
dc.contributor.authorTrichas, M.
dc.contributor.authorTugwell, K.E.
dc.contributor.authorVaccari, M.
dc.contributor.authorValtchanov, I.
dc.contributor.authorVieira, J. D.
dc.contributor.authorVigroux, L.
dc.contributor.authorWard, R.
dc.contributor.authorWright, G.
dc.contributor.authorXu, C.K.
dc.contributor.authorZemcov, M.
dc.date.accessioned2012-03-21T09:00:36Z
dc.date.available2012-03-21T09:00:36Z
dc.date.issued2010-07-01
dc.identifier.citationCooray , A , Amblard , A , Arumugam , V , Wang , L , Auld , R , Aussel , H , Babbedge , T , Blain , A , Bock , J , Boselli , A , Buat , V , Burgarella , D , Castro-Rodriguez , N , Cava , A , Chanial , P , Clements , D L , Conley , A , Conversi , L , Dowell , C D , Dwek , E , Eales , S , Elbaz , D , Farrah , D , Fox , M , Franceschini , A , Gear , W , Glenn , J , Griffin , M , Halpern , M , Hatziminaoglou , E , Ibar , E , Isaak , K , Ivison , R J , Khostovan , A A , Lagache , G , Levenson , L , Lu , N , Madden , S , Maffei , B , Mainetti , G , Marchetti , L , Marsden , G , Mitchell-Wynne , K , Mortier , A M J , Nguyen , H T , O'Halloran , B , Oliver , S J , Omont , A , Page , M J , Panuzzo , P , Papageorgiou , A , Pearson , C P , Perez Fournon , I , Pohlen , M , Rawlings , J I , Raymond , G , Rigopoulou , D , Rizzo , D , Roseboom , I G , Rowan-Robinson , M , Schulz , B , Scott , D , Serra , P , Seymour , N , Shupe , D L , Smith , A J , Stevens , J , Symeonidis , M , Trichas , M , Tugwell , K E , Vaccari , M , Valtchanov , I , Vieira , J D , Vigroux , L , Ward , R , Wright , G , Xu , C K & Zemcov , M 2010 , ' HerMES: Halo occupation number and bias properties of dusty galaxies from angular clustering measurements ' , Astronomy and Astrophysics , vol. 518 , L22 . https://doi.org/10.1051/0004-6361/201014597
dc.identifier.issn0004-6361
dc.identifier.otherPURE: 519683
dc.identifier.otherPURE UUID: c35a2a57-04ad-4631-be0b-6f7010968812
dc.identifier.otherBibtex: urn:860df4c067fa5df8f2c29241daef73b2
dc.identifier.otherScopus: 77957830244
dc.identifier.otherORCID: /0000-0002-4010-8310/work/62747585
dc.identifier.urihttp://hdl.handle.net/2299/8012
dc.description.abstractWe measure the angular correlation function, w(θ), from 0.5 to 30 arcmin of detected sources in two wide fields of the Herschel Multi-tiered Extragalactic Survey (HerMES). Our measurements are consistent with the expected clustering shape from a population of sources that trace the dark matter density field, including non-linear clustering at arcminute angular scales arising from multiple sources that occupy the same dark matter halos. By making use of the halo model to connect the spatial clustering of sources to the dark matter halo distribution, we estimate source bias and halo occupation number for dusty sub-mm galaxies at z ∼ 2. We find that sub-mm galaxies with 250 μm flux densities above 30 mJy reside in dark matter halos with mass above (5±4)×1012 , while (14±8)% of such sources appear as satellites in more massive halos.en
dc.format.extent5
dc.language.isoeng
dc.relation.ispartofAstronomy and Astrophysics
dc.rightsOpen
dc.subjectsubmillimeter: galaxies, large-scale structure of Universe, cosmology: observations, galaxies: evolution, galaxies: high-redshift
dc.titleHerMES: Halo occupation number and bias properties of dusty galaxies from angular clustering measurementsen
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.description.versiontypeFinal Accepted Version
dcterms.dateAccepted2010-07-01
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1051/0004-6361/201014597
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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