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Wiley, Monthly Notice- Royal Astronomical Society -Letters-, 1(453), p. L83-L87

DOI: 10.1093/mnrasl/slv110

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ALMA andHerschelreveal that X-ray-selected AGN and main-sequence galaxies have different star formation rate distributions

Journal article published in 2015 by J. R. Mullaney, D. M. Alexander ORCID, J. Aird, E. Bernhard, E. Daddi ORCID, A. Del Moro, M. Dickinson, D. Elbaz, C. M. Harrison, S. Juneau, D. Liu ORCID, M. Pannella ORCID, D. Rosario, P. Santini ORCID, M. Sargent and other authors.
This paper is available in a repository.
This paper is available in a repository.

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Abstract

Using deep Herschel and ALMA observations, we investigate the star formation rate (SFR) distributions of X-ray-selected active galactic nucleus (AGN) host galaxies at 0.5