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

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        904372.pdf (PDF, 136Kb)
        Author
        Dye, S.
        Dunne, L.
        Eales, S.
        Smith, Daniel
        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.
        Attention
        2299/7906
        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.
        Publication date
        2010
        Published in
        Astronomy and Astrophysics
        Published version
        https://doi.org/10.1051/0004-6361/201014614
        Other links
        http://hdl.handle.net/2299/7906
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