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Cited article:
M. Michałowski , J. Hjorth , D. Watson
A&A, 514 (2010) A67
Published online: 2010-05-28
This article has been cited by the following article(s):
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Herschel-ATLAS: the far-infrared-radio correlation at z < 0.5★
Matt J. Jarvis, D. J. B. Smith, D. G. Bonfield, et al. Monthly Notices of the Royal Astronomical Society 409 (1) 92 (2010) https://doi.org/10.1111/j.1365-2966.2010.17772.x
The dust content of high-zsubmillimeter galaxies revealed byHerschel
P. Santini, R. Maiolino, B. Magnelli, et al. Astronomy and Astrophysics 518 L154 (2010) https://doi.org/10.1051/0004-6361/201014748
A simple approach to the high-redshift sub-millimeter galaxies
Tamon Suwa, Hiroyuki Hirashita and Yoichi Tamura Astrophysics and Space Science 330 (2) 219 (2010) https://doi.org/10.1007/s10509-010-0408-9
MOST SUBMILLIMETER GALAXIES ARE MAJOR MERGERS
H. Engel, L. J. Tacconi, R. I. Davies, et al. The Astrophysical Journal 724 (1) 233 (2010) https://doi.org/10.1088/0004-637X/724/1/233
HerschelATLAS: The cosmic star formation history of quasar host galaxies
S. Serjeant, F. Bertoldi, A. W. Blain, et al. Astronomy and Astrophysics 518 L7 (2010) https://doi.org/10.1051/0004-6361/201014565
A physical model for z∼ 2 dust-obscured galaxies★
Desika Narayanan, Arjun Dey, Christopher C. Hayward, et al. Monthly Notices of the Royal Astronomical Society 407 (3) 1701 (2010) https://doi.org/10.1111/j.1365-2966.2010.16997.x
SUBMILLIMETER GALAXY NUMBER COUNTS AND MAGNIFICATION BY GALAXY CLUSTERS
Marcos Lima, Bhuvnesh Jain, Mark Devlin and James Aguirre The Astrophysical Journal 717 (1) L31 (2010) https://doi.org/10.1088/2041-8205/717/1/L31
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