The mean star formation rates of unobscured QSOs: searching for evidence of suppressed or enhanced star formation

Stanley, F. and Alexander, D.M. and Harrison, C.M. and Rosario, D.J. and Wang, L. and Aird, J.A. and Bourne, N. and Dunne, L. and Dye, S. and Eales, S. and Knudsen, K.K. and Michałowski, M.J. and Valiante, E. and De Zotti, G. and Furlanetto, C. and Ivison, R. and Maddox, S. and Smith, M.W.L. (2017) The mean star formation rates of unobscured QSOs: searching for evidence of suppressed or enhanced star formation. Monthly Notices of the Royal Astronomical Society, 472 (2). pp. 2221-2240. ISSN 0035-8711

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Abstract

We investigate the mean star formation rates (SFRs) in the host galaxies of ∼3000 optically selected quasi-stellar objects (QSOs) from the Sloan Digital Sky Survey within the Herschel-ATLAS fields, and a radio-luminous subsample covering the redshift range of z = 0.2–2.5. Using Wide-field Infrared Survey Explorer (WISE) and Herschel photometry (12–500 μm) we construct composite spectral energy distributions (SEDs) in bins of redshift and active galactic nucleus (AGN) luminosity. We perform SED fitting to measure the mean infrared luminosity due to star formation, removing the contamination from AGN emission. We find that the mean SFRs show a weak positive trend with increasing AGN luminosity. However, we demonstrate that the observed trend could be due to an increase in black hole (BH) mass (and a consequent increase of inferred stellar mass) with increasing AGN luminosity. We compare to a sample of X-ray selected AGN and find that the two populations have consistent mean SFRs when matched in AGN luminosity and redshift. On the basis of the available virial BH masses, and the evolving BH mass to stellar mass relationship, we find that the mean SFRs of our QSO sample are consistent with those of main sequence star-forming galaxies. Similarly the radio-luminous QSOs have mean SFRs that are consistent with both the overall QSO sample and with star-forming galaxies on the main sequence. In conclusion, on average QSOs reside on the main sequence of star-forming galaxies, and the observed positive trend between the mean SFRs and AGN luminosity can be attributed to BH mass and redshift dependencies.

Item Type: Article
Additional Information: This article has been accepted for publication in © 2017 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Schools/Departments: University of Nottingham, UK > Faculty of Science > School of Physics and Astronomy
Identification Number: 10.1093/mnras/stx2121
Depositing User: Eprints, Support
Date Deposited: 20 Dec 2017 13:06
Last Modified: 21 Dec 2017 20:56
URI: http://eprints.nottingham.ac.uk/id/eprint/48822

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