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dc.contributor.authorDye, S.-
dc.contributor.authorHerranz, D.-
dc.contributor.authorLópez-Caniego, M.-
dc.date.accessioned2012-02-22T14:55:31Z-
dc.date.available2012-02-22T14:55:31Z-
dc.date.issued2010-
dc.identifier.citationAstronomy and Astrophysics 518: L10 (2010)es_ES
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/10261/46080-
dc.description5 páginas, 4 figuras.-- Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.-- et al.es_ES
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 steadily out to this redshift. By selecting a sub-group of sources within a fixed luminosity interval where incompleteness effects are minimal, we have measured a smooth increase in the comoving 250 μm luminosity density out to z = 0.2 where it is 3.6+1.4-0.9 times higher than the local value.es_ES
dc.description.sponsorshipS.D. Acknowledges the UK STFC for support.es_ES
dc.language.isoenges_ES
dc.publisherEDP Scienceses_ES
dc.rightsopenAccesses_ES
dc.subjectGalaxies: luminosity function, mass functiones_ES
dc.subjectCosmology: observationses_ES
dc.subjectLarge-scale structure of Universees_ES
dc.titleHerschel-ATLAS: Evolution of the 250 µm luminosity function out to z = 0.5es_ES
dc.typeartículoes_ES
dc.identifier.doihttp://dx.doi.org/10.1051/0004-6361/201014614-
dc.description.peerreviewedPeer reviewedes_ES
dc.relation.publisherversionhttp://dx.doi.org/10.1051/0004-6361/201014614es_ES
dc.identifier.e-issn1432-0746-
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