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dc.contributorVirginia Techen
dc.contributor.authorBurgarella, D.en
dc.contributor.authorGruppioni, C.en
dc.contributor.authorCucciati, O.en
dc.contributor.authorHeinis, S.en
dc.contributor.authorBerta, S.en
dc.contributor.authorBethermin, M.en
dc.contributor.authorBock, J.en
dc.contributor.authorCooray, A.en
dc.contributor.authorDunlop, J. S.en
dc.contributor.authorFarrah, D.en
dc.contributor.authorFranceschini, A.en
dc.contributor.authorLe Floc'h, E.en
dc.contributor.authorLutz, D.en
dc.contributor.authorMagnelli, B.en
dc.contributor.authorNordon, R.en
dc.contributor.authorOliver, S. J.en
dc.contributor.authorPage, M. J.en
dc.contributor.authorPopesso, P.en
dc.contributor.authorPozzi, F.en
dc.contributor.authorRiguccini, L.en
dc.contributor.authorVaccari, M.en
dc.contributor.authorViero, M.en
dc.date.accessioned2013-12-06T13:58:47Zen
dc.date.available2013-12-06T13:58:47Zen
dc.date.issued2013-06en
dc.identifier.citationBurgarella, D. ; Buat, V. ; Gruppioni, C. ; et al., Jun 2013. “Herschel PEP/HerMES: the redshift evolution (0 <= z <= 4) of dust attenuation and of the total (UV plus IR) star formation rate density,” ASTRONOMY & ASTROPHYSICS 554:A70. DOI: 10.1051/0004-6361/201321651en
dc.identifier.issn0004-6361en
dc.identifier.urihttp://hdl.handle.net/10919/24430en
dc.description.abstractUsing new homogeneous luminosity functions (LFs) in the far-ultraviolet (FUV) from VVDS and in the far-infrared (FIR) from Herschel/PEP and Herschel/HerMES, we studied the evolution of the dust attenuation with redshift. With this information, we were able to estimate the redshift evolution of the total (FUV + FIR) star formation rate density (SFRDTOT). By integrating SFRDTOT, we followed the mass building and analyzed the redshift evolution of the stellar mass density (SMD). This article aims at providing a complete view of star formation from the local Universe to z similar to 4 and, using assumptions on earlier star formation history, compares this evolution with previously published data in an attempt to draw a homogeneous picture of the global evolution of star formation in galaxies. Our main conclusions are that: 1) the dust attenuation A(FUV) is found to increase from z = 0 to z similar to 1.2 and then starts to decrease until our last data point at z = 3 : 6; 2) the estimated SFRD confirms published results to z similar to 2. At z > 2, we observe either a plateau or a small increase up to z similar to 3 and then a likely decrease up to z = 3.6; 3) the peak of AFUV is delayed with respect to the plateau of SFRDTOT and a probable origin might be found in the evolution of the bright ends of the FUV and FIR LFs; 4) using assumptions (exponential rise and linear rise with time) for the evolution of the star formation density from z = 3 : 6 to z(form) = 10, we integrated SFRDTOT and obtained a good agreement with the published SMDs.en
dc.description.sponsorshipBMVIT (Austria)en
dc.description.sponsorshipESA-PRODEX (Belgium)en
dc.description.sponsorshipCEA/CNES (France)en
dc.description.sponsorshipDLR (Germany)en
dc.description.sponsorshipASI/INAF (Italy)en
dc.description.sponsorshipCICYT/MCYT (Spain)en
dc.description.sponsorshipCSA (Canada)en
dc.description.sponsorshipNAOC (China)en
dc.description.sponsorshipCEA (France)en
dc.description.sponsorshipCNES (France)en
dc.description.sponsorshipCNRS (France)en
dc.description.sponsorshipASI (Italy)en
dc.description.sponsorshipMCINN (Spain)en
dc.description.sponsorshipSNSB (Sweden)en
dc.description.sponsorshipSTFC (UK)en
dc.description.sponsorshipUKSA (UK)en
dc.description.sponsorshipNASA (USA)en
dc.description.sponsorshipPRIN-INAF 1.06.09.05en
dc.description.sponsorshipASI-INAF I00507/1, I005110en
dc.description.sponsorshipStockholm Observatory (Sweden)en
dc.language.isoen_USen
dc.publisherEDP Sciencesen
dc.rightsIn Copyrighten
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/en
dc.subjectearly Universeen
dc.subjectcosmology: observationsen
dc.subjectgalaxies: star formationen
dc.subjectinfrared: galaxiesen
dc.subjectgalaxies: starbursten
dc.subjectultraviolet: galaxiesen
dc.subjectlyman-break galaxiesen
dc.subjectearly release scienceen
dc.subjectluminosity functionen
dc.subjectformation historyen
dc.subjectforming galaxiesen
dc.subjectdistant galaxiesen
dc.subjectgas accretionen
dc.subjectstellar massen
dc.subjectultravioleten
dc.subjectmultiwavelengthen
dc.subjectAstronomy & Astrophysicsen
dc.titleHerschel PEP/HerMES: the redshift evolution (0 <= z <= 4) of dust attenuation and of the total (UV plus IR) star formation rate densityen
dc.typeArticle - Refereeden
dc.contributor.departmentPhysicsen
dc.identifier.urlhttp://www.aanda.org/articles/aa/pdf/2013/06/aa21651-13.pdfen
dc.date.accessed2013-12-05en
dc.title.serialAstronomy & Astrophysicsen
dc.identifier.doihttps://doi.org/10.1051/0004-6361/201321651en


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