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    First results from HerMES on the evolution of the submillimetre luminosity function

    Access Status
    Open access via publisher
    Authors
    Eales, S.
    Raymond, G.
    Roseboom, I.
    Altieri, B.
    Amblard, A.
    Arumugam, V.
    Auld, R.
    Aussel, H.
    Babbedge, T.
    Blain, A.
    Bock, J.
    Boselli, A.
    Brisbin, D.
    Buat, V.
    Burgarella, D.
    Castro-Rodríguez, N.
    Cava, A.
    Chanial, P.
    Clements, D.
    Conley, A.
    Conversi, L.
    Cooray, A.
    Dowell, C.
    Dwek, E.
    Dye, S.
    Elbaz, D.
    Farrah, D.
    Fox, M.
    Franceschini, A.
    Gear, W.
    Glenn, J.
    González Solares, E.
    Griffin, M.
    Harwit, M.
    Hatziminaoglou, E.
    Huang, J.
    Ibar, E.
    Isaak, K.
    Ivison, R.
    Lagache, G.
    Levenson, L.
    Lonsdale, C.
    Lu, N.
    Madden, S.
    Maffei, B.
    Mainetti, G.
    Marchetti, L.
    Morrison, G.
    Mortier, A.
    Nguyen, H.
    O'Halloran, B.
    Oliver, S.
    Omont, A.
    Owen, F.
    Page, M.
    Pannella, M.
    Panuzzo, P.
    Papageorgiou, A.
    Pearson, C.
    Pérez-Fournon, I.
    Pohlen, M.
    Rawlings, J.
    Rigopoulou, D.
    Rizzo, D.
    Rowan-Robinson, M.
    Sánchez Portal, M.
    Schulz, B.
    Scott, D.
    Seymour, Nick
    Shupe, D.
    Smith, A.
    Stevens, J.
    Strazzullo, V.
    Symeonidis, M.
    Trichas, M.
    Tugwell, K.
    Vaccari, M.
    Valtchanov, I.
    Vigroux, L.
    Wang, L.
    Ward, R.
    Wright, G.
    Xu, C.
    Date
    2010
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Eales, S. and Raymond, G. and Roseboom, I. and Altieri, B. and Amblard, A. and Arumugam, V. and Auld, R. et al. 2010. First results from HerMES on the evolution of the submillimetre luminosity function. Astronomy and Astrophysics. 518 (2).
    Source Title
    Astronomy and Astrophysics
    DOI
    10.1051/0004-6361/201014675
    ISSN
    0004-6361
    School
    Department of Physics and Astronomy
    URI
    http://hdl.handle.net/20.500.11937/37367
    Collection
    • Curtin Research Publications
    Abstract

    We have carried out two extremely deep surveys with SPIRE, one of the two cameras on Herschel, at 250 µm, close to the peak of the far-infrared background. We have used the results to investigate the evolution of the rest-frame 250-µm luminosity function out to z = 2. We find evidence for strong evolution out to z $\simeq$ 1 but evidence for at most weak evolution beyond this redshift. Our results suggest that a significant part of the stars and metals in the universe today were formed at z 1.4 in spiral galaxies. © 2010 ESO.

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