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An extended Hersche...
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Boone, F.Université de Toulouse,University of Toulouse,Centre national de la recherche scientifique (CNRS)
(author)
An extended Herschel drop-out source in the center of AS1063: A normal dusty galaxy at z = 6.1 or SZ substructures?
- Article/chapterEnglish2013
Publisher, publication year, extent ...
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2013-10-30
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EDP Sciences,2013
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electronicrdacarrier
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LIBRIS-ID:oai:research.chalmers.se:98ebfd24-60c4-4933-881e-97d190cb4903
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https://research.chalmers.se/publication/188935URI
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https://doi.org/10.1051/0004-6361/201322552DOI
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Language:English
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Summary in:English
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Subject category:art swepub-publicationtype
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Subject category:ref swepub-contenttype
Notes
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In the course of our 870 μm APEX/LABOCA follow-up of the Herschel Lensing Survey we have detected a source in AS1063 (RXC J2248.7-4431) that has no counterparts in any of the Herschel PACS/SPIRE bands, it is a Herschel "drop-out" with S870=S500 ≥ 0:5. The 870 μm emission is extended and centered on the brightest cluster galaxy, suggesting either a multiply imaged background source or substructure in the Sunyaev-Zel'dovich increment due to inhomogeneities in the hot cluster gas of this merging cluster. We discuss both interpretations with emphasis on the putative lensed source. Based on the observed properties and on our lens model we find that this source may be the first submillimeter galaxy (SMG) with a moderate far-infrared (FIR) luminosity (LFIR. © ESO 2013.
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Clément, B.University of Arizona
(author)
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Richard, J.Université de Lyon
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Schaerer, D.Centre national de la recherche scientifique (CNRS),Université de Genève,University of Geneva
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Lutz, D.Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
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Weiß, A.Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
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Zemcov, M.California Institute of Technology (Caltech)
(author)
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Egami, E.University of Arizona
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Rawle, T.D.European Space Astronomy Centre (ESAC)
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Walth, G.L.University of Arizona
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Kneib, J.P.J.P.Laboratoire d'Astrophysique de Marseille,Ecole Polytechnique Federale de Lausanne (EPFL),Swiss Federal Institute of Technology in Lausanne (EPFL)
(author)
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Combes, F.LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres, France
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Smail, I.A.N.Durham University
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Swinbank, A.M.Durham University
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Altiéri, B.European Space Astronomy Centre (ESAC)
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Blain, A.W.University Of Leicester
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Chapman, S.C.Dalhousie University
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Dessauges-Zavadsky, M.Université de Genève,University of Geneva
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Ivison, R.J.University of Edinburgh
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Knudsen, Kirsten Kraiberg,1976Chalmers tekniska högskola,Chalmers University of Technology(Swepub:cth)kraiberg
(author)
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Omont, A.A.
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Pelló, R.Université de Toulouse,University of Toulouse,Centre national de la recherche scientifique (CNRS)
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Pérez-González, P.G.P.Universidad Complutense de Madrid,Complutense University
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Valtchanov, I.European Space Astronomy Centre (ESAC)
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van der Werf, P.P.Universiteit Leiden (UL),Leiden University (UL)
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Zamojski, M.A.Université de Genève,University of Geneva
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Université de ToulouseCentre national de la recherche scientifique (CNRS)
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In:Astronomy and Astrophysics: EDP Sciences559, s. L1-0004-63611432-0746
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Boone, F.
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Clément, B.
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Richard, J.
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Schaerer, D.
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Lutz, D.
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Weiß, A.
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Zemcov, M.
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Egami, E.
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Rawle, T.D.
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Walth, G.L.
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Kneib, J.P.J.P.
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Combes, F.
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Smail, I.A.N.
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Swinbank, A.M.
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Altiéri, B.
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Blain, A.W.
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Chapman, S.C.
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Dessauges-Zavads ...
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Ivison, R.J.
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Knudsen, Kirsten ...
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Omont, A.A.
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Pelló, R.
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Pérez-González, ...
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Valtchanov, I.
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van der Werf, P. ...
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Zamojski, M.A.
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