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The far-infrared/submillimeter properties of galaxies located behind the Bullet cluster

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Pérez González, Pablo Guillermo y otros, ... (2010) The far-infrared/submillimeter properties of galaxies located behind the Bullet cluster. Astronomy & Astrophysics, 518 . ISSN 0004-6361

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URL Oficial: http://dx.doi.org/10.1051/0004-6361/201014693


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Resumen

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.


Tipo de documento:Artículo
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© ESO, 2010.
Artículo firmado por 48 autores.
We thank Ben Weiner and David Elbaz for their valuable comments and help with our computations. This work is based in part on observations made with Herschel, a European Space Agency Cornerstone Mission with significant participation by NASA. Support for this work was provided by NASA through an award issued by JPL/Caltech.

Palabras clave:Star-forming galaxies; Submillimeter galaxies; Redshift deadlock; 1e0657-56; Evolution; Breaking; Bright
Materias:Ciencias > Física > Astrofísica
Ciencias > Física > Astronomía
Código ID:38557
Depositado:21 Jul 2016 15:55
Última Modificación:21 Jul 2016 15:55

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