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    HerMES: The submillimeter spectral energy distributions of Herschel/SPIRE-detected galaxies

    Access Status
    Open access via publisher
    Authors
    Schulz, B.
    Pearson, C.
    Clements, D.
    Altieri, B.
    Amblard, A.
    Arumugam, V.
    Auld, R.
    Aussel, H.
    Babbedge, T.
    Blain, A.
    Bock, J.
    Boselli, A.
    Buat, V.
    Burgarella, D.
    Castro-Rodríguez, N.
    Cava, A.
    Chanial, P.
    Conley, A.
    Conversi, L.
    Cooray, A.
    Dowell, C.
    Dwek, E.
    Eales, S.
    Elbaz, D.
    Fox, M.
    Franceschini, A.
    Gear, W.
    Giovannoli, E.
    Glenn, J.
    Griffin, M.
    Halpern, M.
    Hatziminaoglou, E.
    Ibar, E.
    Isaak, K.
    Ivison, R.
    Lagache, G.
    Levenson, L.
    Lu, N.
    Madden, S.
    Maffei, B.
    Mainetti, G.
    Marchetti, L.
    Marsden, G.
    Mortier, A.
    Nguyen, H.
    O'Halloran, B.
    Oliver, S.
    Omont, A.
    Page, M.
    Panuzzo, P.
    Papageorgiou, A.
    Pérez-Fournon, I.
    Pohlen, M.
    Rangwala, N.
    Rawlings, J.
    Raymond, G.
    Rigopoulou, D.
    Rizzo, D.
    Roseboom, I.
    Rowan-Robinson, M.
    Sánchez Portal, M.
    Scott, D.
    Seymour, Nick
    Shupe, D.
    Smith, A.
    Stevens, J.
    Symeonidis, M.
    Trichas, M.
    Tugwell, K.
    Vaccari, M.
    Valiante, E.
    Valtchanov, I.
    Vigroux, L.
    Wang, L.
    Ward, R.
    Wright, G.
    Xu, C.
    Zemcov, M.
    Date
    2010
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Schulz, B. and Pearson, C. and Clements, D. and Altieri, B. and Amblard, A. and Arumugam, V. and Auld, R. et al. 2010. HerMES: The submillimeter spectral energy distributions of Herschel/SPIRE-detected galaxies. Astronomy and Astrophysics. 518 (2).
    Source Title
    Astronomy and Astrophysics
    DOI
    10.1051/0004-6361/201014673
    ISSN
    0004-6361
    School
    Department of Physics and Astronomy
    URI
    http://hdl.handle.net/20.500.11937/32233
    Collection
    • Curtin Research Publications
    Abstract

    We present colours of sources detected with the Herschel/SPIRE instrument in deep extragalactic surveys of the Lockman Hole, Spitzer-FLS, and GOODS-N fields in three photometric bands at 250, 350 and 500 µm. We compare these with expectations from the literature and discuss associated uncertainties and biases in the SPIRE data. We identify a 500 µm flux limited selection of sources from the HerMES point source catalogue that appears free from neighbouring/blended sources in all three SPIRE bands. We compare the colours with redshift tracks of various contemporary models. Based on these spectral templates we show that regions corresponding to specific population types and redshifts can be identified better in colour-flux space. The redshift tracks as well as the colour-flux plots imply a majority of detected objects with redshifts at 1 < z < 3.5, somewhat depending on the group of model SEDs used. We also find that a population of sources with S250/S 350 < 0.8 at fluxes above 50 mJy as observed by SPIRE are not well represented by contemporary models and could consist of a mix of cold and lensed galaxies. © 2010 ESO.

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