Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/11507
Title: The Deep SPIRE HerMES Survey: spectral energy distributions and their astrophysical indications at high redshift
Authors: Harwit, M.
Altieri, B.
Amblard, A.
Arumugam, V.
Aussel, H.
Babbedge, T.
Blain, A.
Bock, J.
Boselli, A.
Buat, V.
Castro-Rodriguez, N.
Cava, A.
Chanial, P.
Clements, D. L.
Conley, A.
Conversi, L.
Cooray, A.
Dowell, C. D.
Dwek, E.
Eales, S.
Elbaz, D.
Fox, M.
Franceschini, A.
Gear, W.
Glenn, J.
Griffin, M.
Halpern, M.
Hatziminaoglou, E.
Ibar, E.
Isaak, K.
Ivison, R. J.
Lagache, G.
Levenson, L.
Lonsdale, C. J.
Lu, N.
Madden, S.
Maffei, B.
Mainetti, G.
Marchetti, L.
Morrison, G. E.
Nguyen, H. T.
O'Halloran, B.
Oliver, S. J.
Omont, A.
Owen, F. N.
Pannella, M.
Panuzzo, P.
Papageorgiou, A.
Pearson, C. P.
Perez-Fournon, I.
Pohlen, M.
Rizzo, D.
Roseboom, I. G.
Rowan-Robinson, M.
Sanchez Portal M.
Schulz, B.
Seymour, N.
Shupe, D. L.
Smith, A. J.
Stevens, J. A.
Strazzullo, V.
Symeonidis, M.
Trichas, M.
Tugwell, K. E.
Vaccari, M.
Valtchanov, I.
Vigroux, L.
Wang, L.
Ward, R.
Wright, G.
Xu, C. K.
Zemcov, M.
First Published: 21-Nov-2010
Publisher: Oxford University Press (OUP)
Oxford University Press (OUP)
Citation: Monthly Notices of the Royal Astronomical Society , 2010, 409 (1), pp. 66-74
Abstract: The Spectral and Photometric Imaging Receiver on-board Herschel has been carrying out deep extragalactic surveys, one of the aims of which is to establish spectral energy distributions of individual galaxies spanning the infrared/submillimetre (IR/SMM) wavelength region. We report observations of the IR/SMM emission from the Lockman North field and Great Observatories Origins Deep Survey Field-North. Because galaxy images in the wavelength range covered by Herschel generally represent a blend with contributions from neighbouring galaxies, we present sets of galaxies in each field, especially free of blending at 250, 350 and 500 μm. We identify the cumulative emission of these galaxies and the fraction of the FIR cosmic background radiation they contribute. Our surveys reveal a number of highly luminous galaxies at redshift z≲ 3 and a novel relationship between IR and visible emission that shows a dependence on luminosity and redshift.
DOI Link: 10.1111/j.1365-2966.2010.17643.x
ISSN: 0035-8711
Links: http://hdl.handle.net/2381/11507
http://mnras.oxfordjournals.org/content/409/1/66
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2010 the authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. Deposited with reference to the publisher’s archiving policy available on the SHERPA/RoMEO website.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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