Herschel-ATLAS: Evolution of the 250 µm luminosity function out to z = 0.5
dc.contributor.author | Dye, S. | |
dc.contributor.author | Dunne, L. | |
dc.contributor.author | Eales, S. | |
dc.contributor.author | Smith, Daniel | |
dc.contributor.author | Amblard, A. | |
dc.contributor.author | Auld, R. | |
dc.contributor.author | Baes, M. | |
dc.contributor.author | Baldry, I.K. | |
dc.contributor.author | Bamford, S. | |
dc.contributor.author | Blain, A.W. | |
dc.contributor.author | Bonfield, D. | |
dc.contributor.author | Bremer, M. | |
dc.contributor.author | Burgarella, D. | |
dc.contributor.author | Buttiglione, S. | |
dc.contributor.author | Cameron, E. | |
dc.contributor.author | Cava, A. | |
dc.contributor.author | Clements, D. | |
dc.contributor.author | Cooray, A. | |
dc.contributor.author | Croom, S. | |
dc.contributor.author | Dariush, A. | |
dc.contributor.author | de Zotti, G. | |
dc.contributor.author | Driver, S. | |
dc.contributor.author | Dunlop, J.S. | |
dc.contributor.author | Frayer, D. | |
dc.contributor.author | Fritz, J. | |
dc.contributor.author | Gardner, J.P. | |
dc.contributor.author | Gomez, H.L. | |
dc.contributor.author | Gonzalez-Nuevo, J. | |
dc.contributor.author | Herranz, D. | |
dc.contributor.author | Hill, D. | |
dc.contributor.author | Hopkins, A. | |
dc.contributor.author | Ibar, E. | |
dc.contributor.author | Ivison, R.J. | |
dc.contributor.author | Jarvis, M.J. | |
dc.contributor.author | Jones, D.H. | |
dc.contributor.author | Kelvin, L. | |
dc.contributor.author | Lagache, G. | |
dc.contributor.author | Leeuw, L. | |
dc.contributor.author | Liske, J. | |
dc.contributor.author | Lopez-Caniego, M. | |
dc.contributor.author | Loveday, J. | |
dc.contributor.author | Maddox, S. | |
dc.contributor.author | Michalowski, M. | |
dc.contributor.author | Negrello, M. | |
dc.contributor.author | Norberg, P. | |
dc.contributor.author | Page, M.J. | |
dc.contributor.author | Parkinson, H. | |
dc.contributor.author | Pascale, E. | |
dc.contributor.author | Peacock, J.A. | |
dc.contributor.author | Pohlen, M. | |
dc.contributor.author | Popescu, C. | |
dc.contributor.author | Prescott, M. | |
dc.contributor.author | Rigopoulou, D. | |
dc.contributor.author | Robotham, A. | |
dc.contributor.author | Rigby, E. | |
dc.contributor.author | Rodighiero, G. | |
dc.contributor.author | Samui, S. | |
dc.contributor.author | Scott, D. | |
dc.contributor.author | Serjeant, S. | |
dc.contributor.author | Sharp, R.G. | |
dc.contributor.author | Sibthorpe, B. | |
dc.contributor.author | Temi, P. | |
dc.contributor.author | Thompson, M.A. | |
dc.contributor.author | Tuffs, R. | |
dc.contributor.author | Valtchanov, I. | |
dc.contributor.author | van der Werf, P. | |
dc.contributor.author | van Kampen, E. | |
dc.contributor.author | Verma, A. | |
dc.date.accessioned | 2012-03-07T11:00:06Z | |
dc.date.available | 2012-03-07T11:00:06Z | |
dc.date.issued | 2010 | |
dc.identifier.citation | Dye , S , Dunne , L , Eales , S , Smith , D , Amblard , A , Auld , R , Baes , M , Baldry , I K , Bamford , S , Blain , A W , Bonfield , D , Bremer , M , Burgarella , D , Buttiglione , S , Cameron , E , Cava , A , Clements , D , Cooray , A , Croom , S , Dariush , A , de Zotti , G , Driver , S , Dunlop , J S , Frayer , D , Fritz , J , Gardner , J P , Gomez , H L , Gonzalez-Nuevo , J , Herranz , D , Hill , D , Hopkins , A , Ibar , E , Ivison , R J , Jarvis , M J , Jones , D H , Kelvin , L , Lagache , G , Leeuw , L , Liske , J , Lopez-Caniego , M , Loveday , J , Maddox , S , Michalowski , M , Negrello , M , Norberg , P , Page , M J , Parkinson , H , Pascale , E , Peacock , J A , Pohlen , M , Popescu , C , Prescott , M , Rigopoulou , D , Robotham , A , Rigby , E , Rodighiero , G , Samui , S , Scott , D , Serjeant , S , Sharp , R G , Sibthorpe , B , Temi , P , Thompson , M A , Tuffs , R , Valtchanov , I , van der Werf , P , van Kampen , E & Verma , A 2010 , ' Herschel-ATLAS: Evolution of the 250 µm luminosity function out to z = 0.5 ' , Astronomy and Astrophysics , vol. 518 , L10 . https://doi.org/10.1051/0004-6361/201014614 | |
dc.identifier.issn | 0004-6361 | |
dc.identifier.other | dspace: 2299/4995 | |
dc.identifier.other | ORCID: /0000-0001-5392-909X/work/30970847 | |
dc.identifier.other | ORCID: /0000-0001-9708-253X/work/69424325 | |
dc.identifier.uri | http://hdl.handle.net/2299/7906 | |
dc.description | Original article can be found at: http://www.aanda.org/ Copyright The European Southern Observatory | |
dc.description.abstract | 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 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. | en |
dc.format.extent | 139319 | |
dc.language.iso | eng | |
dc.relation.ispartof | Astronomy and Astrophysics | |
dc.title | Herschel-ATLAS: Evolution of the 250 µm luminosity function out to z = 0.5 | en |
dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
dc.contributor.institution | School of Physics, Engineering & Computer Science | |
dc.contributor.institution | Department of Physics, Astronomy and Mathematics | |
dc.description.status | Peer reviewed | |
rioxxterms.versionofrecord | 10.1051/0004-6361/201014614 | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true |