M. Rex
The far-infrared/submillimeter properties of galaxies located behind the Bullet cluster
Rex, M.; Rawle, T.D.; Egami, E.; Pérez-Gonzá&lez, P.G.; Zemcov, M.; Aretxaga, I.; Chung, S.M.; Fadda, D.; Gonzalez, A.H.; Hughes, D.H.; Horellou, C.; Johansson, D.; Kneib, J.-P.; Richard, J.; Altieri, B.; Fiedler, A.K.; Pereira, M.J.; Rieke, G.H.; Smail, I.; Valtchanov, I.; Blain, A.W.; Bock, J.J.; Boone, F.; Bridge, C.R.; Clement, B.; Combes, F.; Dowell, C.D.; Dessauges-Zavadsky, M.; Ilbert, O.; Ivison, R.J.; Jauzac, M.; Lutz, D.; Omont, A.; Pelló, R.; Rodighiero, G.; Schaerer, D.; Smith, G.P.; Walth, G.L.; van der Werf, P.; Werner, M.W.; Austermann, J.E.; Ezawa, H.; Kawabe, R.; Kohno, K.; Perera, T.A.; Scott, K.S.; Wilson, G.W.; Yun, M.S.
Authors
T.D. Rawle
E. Egami
P.G. Pérez-Gonzá&lez
M. Zemcov
I. Aretxaga
S.M. Chung
D. Fadda
A.H. Gonzalez
D.H. Hughes
C. Horellou
D. Johansson
J.-P. Kneib
J. Richard
B. Altieri
A.K. Fiedler
M.J. Pereira
G.H. Rieke
Professor Ian Smail ian.smail@durham.ac.uk
Emeritus Professor
I. Valtchanov
A.W. Blain
J.J. Bock
F. Boone
C.R. Bridge
B. Clement
F. Combes
C.D. Dowell
M. Dessauges-Zavadsky
O. Ilbert
R.J. Ivison
M. Jauzac
D. Lutz
A. Omont
R. Pelló
G. Rodighiero
D. Schaerer
G.P. Smith
G.L. Walth
P. van der Werf
M.W. Werner
J.E. Austermann
H. Ezawa
R. Kawabe
K. Kohno
T.A. Perera
K.S. Scott
G.W. Wilson
M.S. Yun
Abstract
The Herschel Lensing Survey (HLS) takes advantage of gravitational lensing by massive galaxy clusters to sample a population of high-redshift galaxies which are too faint to be detected above the confusion limit of current far-infrared/submillimeter telescopes. Measurements from 100–500 μm bracket the peaks of the far-infrared spectral energy distributions of these galaxies, characterizing their infrared luminosities and star formation rates. We introduce initial results from our science demonstration phase observations, directed toward the Bullet cluster (1E0657-56). By combining our observations with LABOCA 870 μm and AzTEC 1.1 mm data we fully constrain the spectral energy distributions of 19 MIPS 24 μm-selected galaxies which are located behind the cluster. We find that their colors are best fit using templates based on local galaxies with systematically lower infrared luminosities. This suggests that our sources are not like local ultra-luminous infrared galaxies in which vigorous star formation is contained in a compact highly dust-obscured region. Instead, they appear to be scaled up versions of lower luminosity local galaxies with star formation occurring on larger physical scales.
Citation
Rex, M., Rawle, T., Egami, E., Pérez-Gonzá&lez, P., Zemcov, M., Aretxaga, I., …Yun, M. (2010). The far-infrared/submillimeter properties of galaxies located behind the Bullet cluster. Astronomy & Astrophysics, 518, Article L13. https://doi.org/10.1051/0004-6361/201014693
Journal Article Type | Article |
---|---|
Publication Date | Jul 1, 2010 |
Deposit Date | May 28, 2013 |
Publicly Available Date | Mar 29, 2024 |
Journal | Astronomy and astrophysics. |
Print ISSN | 0004-6361 |
Electronic ISSN | 1432-0746 |
Publisher | EDP Sciences |
Peer Reviewed | Peer Reviewed |
Volume | 518 |
Article Number | L13 |
DOI | https://doi.org/10.1051/0004-6361/201014693 |
Keywords | Infrared, Galaxies, Submillimeter, Evolution, High-redshift, Gravitational lensing. |
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Copyright Statement
The original publication is available at http://www.afs-journal.org
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