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Submillimeter galaxies behind the Bullet cluster (1E 0657-56)

Authors :
Johansson, D.
Horellou, C.
Sommer, M. W.
Basu, K.
Bertoldi, F.
Birkinshaw, M.
Lancaster, K.
Lopez-Cruz, O.
Quintana, H.
Source :
Astronomy and Astrophysics; May 2010, Vol. 514 Issue: 1
Publication Year :
2010

Abstract

Context. Clusters of galaxies are effective gravitational lenses able to magnify background galaxies and making it possible to probe the fainter part of the galaxy population. Submillimeter galaxies, which are believed to be star-forming galaxies at typical redshifts of 2 to 3, are a major contaminant to the extended Sunyaev-Zeldovich (SZ) signal of galaxy clusters. For a proper quantification of the SZ signal the contribution of submillimeter galaxies needs to be quantified.

Details

Language :
English
ISSN :
00046361 and 14320746
Volume :
514
Issue :
1
Database :
Supplemental Index
Journal :
Astronomy and Astrophysics
Publication Type :
Periodical
Accession number :
ejs53145850
Full Text :
https://doi.org/10.1051/0004-6361/200913833