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

Mullaney, J.R.; Alexander, D.M.; Aird, J.; Bernhard, E.; Daddi, E.; Del Moro, A.; Dickinson, M.; Elbaz, D.; Harrison, C.M.; Juneau, S.; Liu, D.; Pannella, M.; Rosario, D.; Santini, P.; Sargent, M.; Schreiber, C.; Simpson, J.; Stanley, F.

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


Authors

J.R. Mullaney

J. Aird

E. Bernhard

E. Daddi

A. Del Moro

M. Dickinson

D. Elbaz

C.M. Harrison

S. Juneau

D. Liu

M. Pannella

D. Rosario

P. Santini

M. Sargent

C. Schreiber

J. Simpson

F. Stanley



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 < z < 1.5 and 1.5 < z < 4, comparing them to that of normal, star-forming (i.e. ‘main-sequence’, or MS) galaxies. We find that 34–55 per cent of AGNs in our sample have SFRs at least a factor of 2 below that of the average MS galaxy, compared to ≈15 per cent of all MS galaxies, suggesting significantly different SFR distributions. Indeed, when both are modelled as lognormal distributions, the mass and redshift-normalized SFR distributions of X-ray AGNs are roughly twice as broad, and peak ≈0.4 dex lower, than that of MS galaxies. However, like MS galaxies, the normalized SFR distribution of AGNs in our sample appears not to evolve with redshift. Despite X-ray AGNs and MS galaxies having different SFR distributions, the linear-mean SFR of AGNs derived from our distributions is remarkably consistent with that of MS galaxies, and thus with previous results derived from stacked Herschel data. This apparent contradiction is due to the linear-mean SFR being biased by bright outliers, and thus does not necessarily represent a true characterization of the typical SFR of X-ray AGNs.

Citation

Mullaney, J., Alexander, D., Aird, J., Bernhard, E., Daddi, E., Del Moro, A., …Stanley, F. (2015). ALMA and Herschel reveal that X-ray-selected AGN and main-sequence galaxies have different star formation rate distributions. Monthly Notices of the Royal Astronomical Society: Letters, 453(1), L83-L87. https://doi.org/10.1093/mnrasl/slv110

Journal Article Type Article
Acceptance Date Jul 29, 2015
Online Publication Date Aug 25, 2015
Publication Date Oct 11, 2015
Deposit Date May 31, 2016
Publicly Available Date Jun 15, 2016
Journal Monthly Notices of the Royal Astronomical Society: Letters
Electronic ISSN 1745-3933
Publisher Oxford University Press
Peer Reviewed Peer Reviewed
Volume 453
Issue 1
Pages L83-L87
DOI https://doi.org/10.1093/mnrasl/slv110
Related Public URLs http://adsabs.harvard.edu/abs/2015MNRAS.453L..83M

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Copyright Statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society: Letters ©: 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.







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