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Fundamental differences in the properties of red and blue quasars: measuring the reddening and accretion properties with X-shooter

Fawcett, VA; Alexander, DM; Rosario, DJ; Klindt, L; Lusso, E; Morabito, LK; Calistro Rivera, G

Fundamental differences in the properties of red and blue quasars: measuring the reddening and accretion properties with X-shooter Thumbnail


Authors

VA Fawcett

DJ Rosario

L Klindt

E Lusso

G Calistro Rivera



Abstract

We have recently found fundamental differences in the radio properties of red quasars when compared to typical blue quasars. In this paper, we use data from the X-shooter spectrograph on the Very Large Telescope, providing spectral coverage from ∼3000–25 000 Å, of a sample of 40 red and blue luminous quasars at 1.45 < z < 1.65 to explore the connections between the radio, emission-line, and accretion-disc properties. We fit various dust-extinction curves to the data and find that dust reddening can fully explain the observed colours for the majority of the red quasars in our sample, with moderate extinctions ranging from AV ∼ 0.06–0.7 mag. We confront our spectra with a simple thin accretion-disc model and find this can describe the continua of both the blue and red quasars, once corrected for dust extinction; we also find no significant differences in the accretion properties. We detect ionized outflows in a number of red and blue quasars, but do not find any significant evidence that they are more prevalent in the red quasar population. Overall our findings imply that the radio emission is more closely connected to circumnuclear/ISM opacity rather than accretion disc or outflow differences.

Journal Article Type Article
Acceptance Date Mar 29, 2022
Online Publication Date Apr 13, 2022
Publication Date 2022-06
Deposit Date Jun 1, 2022
Publicly Available Date Jun 1, 2022
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Royal Astronomical Society
Peer Reviewed Peer Reviewed
Volume 513
Issue 1
Pages 1254-1274
DOI https://doi.org/10.1093/mnras/stac945
Public URL https://durham-repository.worktribe.com/output/1202006

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Copyright Statement
This article has been accepted for publication in Monthly notices of the Royal Astronomical Society. ©: 2022 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.






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