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Herschel-ATLAS*: Evolution of the 250 μm luminosity function out to z = 0.5

Dye, S.; Dunne, L.; Eales, S.; Smith, D. J. B.; Amblard, A.; Auld, R.; Baes, M.; Baldry, I. K.; Bamford, Steven P.; Blain, A. W.; Sharp, Robert; Rodighiero, G.

Description

We have determined the luminosity function of 250 μm-selected galaxies detected in the ∼14 deg2 science demonstration region of the Herschel-ATLAS project out to a redshift of z = 0.5. Our findings very clearly show that the luminosity function evolves

dc.contributor.authorDye, S.
dc.contributor.authorDunne, L.
dc.contributor.authorEales, S.
dc.contributor.authorSmith, D. J. B.
dc.contributor.authorAmblard, A.
dc.contributor.authorAuld, R.
dc.contributor.authorBaes, M.
dc.contributor.authorBaldry, I. K.
dc.contributor.authorBamford, Steven P.
dc.contributor.authorBlain, A. W.
dc.contributor.authorSharp, Robert
dc.contributor.authorRodighiero, G.
dc.date.accessioned2015-12-13T22:43:47Z
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/79358
dc.description.abstractWe have determined the luminosity function of 250 μm-selected galaxies detected in the ∼14 deg2 science demonstration region of the Herschel-ATLAS project out to a redshift of z = 0.5. Our findings very clearly show that the luminosity function evolves
dc.publisherSpringer
dc.sourceAstronomy and Astrophysics
dc.subjectKeywords: Cosmology: observation; HERSCHEL; Large scale structure of universe; Luminosity functions; Red shift; Cosmology; Galaxies; Luminance Cosmology: observations; Galaxies: luminosity function, mass function; Large-scale structure of Universe
dc.titleHerschel-ATLAS*: Evolution of the 250 μm luminosity function out to z = 0.5
dc.typeJournal article
local.description.notesImported from ARIES
local.identifier.citationvolume518
dc.date.issued2010
local.identifier.absfor020103 - Cosmology and Extragalactic Astronomy
local.identifier.ariespublicationf5625xPUB7817
local.type.statusPublished Version
local.contributor.affiliationDye, S, Cardiff University
local.contributor.affiliationDunne, L, University of Nottingham
local.contributor.affiliationEales, S, Cardiff University
local.contributor.affiliationSmith, D J B, University of Nottingham
local.contributor.affiliationAmblard, A, University of California
local.contributor.affiliationAuld, R, Cardiff University
local.contributor.affiliationBaes, M, Ghent University
local.contributor.affiliationBaldry, I. K., Liverpool John Moores University
local.contributor.affiliationBamford, Steven P., University of Nottingham
local.contributor.affiliationBlain, A W, California Institute of Technology
local.contributor.affiliationSharp, Robert, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationRodighiero, G, Universita di Padova
local.description.embargo2037-12-31
local.bibliographicCitation.issue1
local.bibliographicCitation.startpageL10
local.identifier.doi10.1051/0004-6361/201014614
dc.date.updated2016-02-24T09:37:25Z
local.identifier.scopusID2-s2.0-77954767657
CollectionsANU Research Publications

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