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19 April 2024

» arxiv » 1009.1371

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The Deep SPIRE HerMES Survey: Spectral Energy Distributions and their Astrophysical Indications at High Redshift
D. Brisbin ; M. Harwit ; B. Altieri ; A. Amblard ; V. Arumugam ; H. Aussel ; T. Babbedge ; A. Blain ; J. Bock ; A. Boselli ; V. Buat ; N. Castro-Rodríguez ; A. Cava ; P. Chanial ; D.L. Clements ; A. Conley ; L. Conversi ; A. Cooray ; C.D. Dowell ; E. Dwek ; S. Eales ; D. Elbaz ; M. Fox ; A. Franceschini ; W. Gear ; J. Glenn ; M. Griffin ; M. Halpern ; E. Hatziminaoglou ; E. Ibar ; K. Isaak ; R.J. Ivison ; G. Lagache ; L. Levenson ; Carol J. Lonsdale ; N. Lu ; S. Madden ; B. Maï¬€ei ; G. Mainetti ; L. Marchetti ; G.E. Morrison ; H.T. Nguyen ; B. Oâ€™Halloran ; S.J. Oliver ; A. Omont ; F.N. Owen ; M. Pannella ; P. Panuzzo ; A. Papageorgiou ; C.P. Pearson ; I. Pérez-Fournon ; M. Pohlen ; D. Rizzo ; I.G. Roseboom ; M. Rowan-Robinson ; M. Sánchez Portal ; B. Schulz ; N. Seymour ; D.L. Shupe ; A.J. Smith ; J.A. Stevens ; V. Strazzullo ; M. Symeonidis ; M. Trichas ; K.E. Tugwell ; M. Vaccari ; I. Valtchanov ; L. Vigroux ; L. Wang ; R. Ward ; G. Wright ; C.K. Xu ; M. Zemcov ;
Date:	7 Sep 2010
Abstract:	The Spectral and Photometric Imaging Receiver (SPIRE) on Herschel has been carrying out deep extragalactic surveys, one of whose aims is to establish spectral energy distributions (SED)s of individual galaxies spanning the infrared/submillimeter (IR/SMM) wavelength region. We report observations of the (IR/SMM) emission from the Lockman North ﬁeld (LN) and Great Observatories Origins Deep Survey ﬁeld North (GOODS-N). Because galaxy images in the wavelength range covered by Herschel generally represent a blend with contributions from neighboring galaxies, we present sets of galaxies in each ﬁeld especially free of blending at 250, 350, and 500 microns. We identify the cumulative emission of these galaxies and the fraction of the far infrared cosmic background radiation they contribute. Our surveys reveal a number of highly luminous galaxies at redshift z ∼< 3 and a novel relationship between infrared and visible emission that shows a dependence on luminosity and redshift.
Source:	arXiv, 1009.1371
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