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dc.contributor.authorHickinbottom, S.
dc.contributor.authorSimpson, C.J.
dc.contributor.authorJames, P.A.
dc.contributor.authorIbar, E.
dc.contributor.authorCarter, D.
dc.contributor.authorBoselli, A.
dc.contributor.authorCollins, C.A.
dc.contributor.authorDavies, J.I.
dc.contributor.authorDunne, L.
dc.contributor.authorEales, S.
dc.contributor.authorFuller, C.
dc.contributor.authorMobasher, B.
dc.contributor.authorPeletier, R.F.
dc.contributor.authorPhillipps, S.
dc.contributor.authorSmith, Daniel
dc.contributor.authorSmith, R.J.
dc.contributor.authorValentijn, E.A.
dc.date.accessioned2015-03-24T12:03:42Z
dc.date.available2015-03-24T12:03:42Z
dc.date.issued2014-08-01
dc.identifier.citationHickinbottom , S , Simpson , C J , James , P A , Ibar , E , Carter , D , Boselli , A , Collins , C A , Davies , J I , Dunne , L , Eales , S , Fuller , C , Mobasher , B , Peletier , R F , Phillipps , S , Smith , D , Smith , R J & Valentijn , E A 2014 , ' A surprising consistency between the far-infrared galaxy luminosity functions of the field and Coma ' , Monthly Notices of the Royal Astronomical Society , vol. 442 , no. 2 , pp. 1286-1293 . https://doi.org/10.1093/mnras/stu924
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 8295411
dc.identifier.otherPURE UUID: f0fd2ee6-57a9-49d2-a1cc-57f62e9e8921
dc.identifier.otherBibtex: urn:d718e0910e03f3d7bfe1f53d7c1814f9
dc.identifier.otherScopus: 84903187794
dc.identifier.otherORCID: /0000-0001-9708-253X/work/69424288
dc.identifier.urihttp://hdl.handle.net/2299/15704
dc.descriptionDate of Acceptance: 06/05/2014
dc.description.abstractWe present new deep images of the Coma Cluster from the ESA Herschel Space Observatory at wavelengths of 70, 100 and 160 μm, covering an area of 1.75 × 1.0 square degrees encompassing the core and south-west infall region. Our data display an excess of sources at flux densities above 100 mJy compared to blank-field surveys, as expected. We use extensive optical spectroscopy of this region to identify cluster members and hence produce cluster luminosity functions in all three photometric bands. We compare our results to the local field galaxy luminosity function, and the luminosity functions from the Herschel Virgo Cluster Survey. We find consistency between the shapes of the Coma and field galaxy luminosity functions at all three wavelengths; however, we do not find the same level of agreement with that of the Virgo Clusteren
dc.format.extent8
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.subjectgalaxies: clusters: individual: Coma, galaxies: luminosity function, mass function, infrared: galaxies
dc.titleA surprising consistency between the far-infrared galaxy luminosity functions of the field and Comaen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1093/mnras/stu924
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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