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The star formation rates of QSOs

Symeonidis, M; Maddox, N; Jarvis, MJ; Michalowski, MJ; Andreani, P; Clements, DL; De Zotti, G; ... Vaccari, M; + view all (2022) The star formation rates of QSOs. Monthly Notices of the Royal Astronomical Society , 514 (3) pp. 4450-4464. 10.1093/mnras/stac1359. Green open access

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Abstract

We examine the far-infrared (FIR) properties of a sample of 5391 optically selected QSOs in the 0.5 < z < 2.65 redshift range down to log [νL_{ν}, 2500(erg s^{−1})] > 44.7, using SPIRE data from Herschel-ATLAS. We split the sample in a grid of 74 luminosity–redshift bins and compute the average optical–IR spectral energy distribution (SED) in each bin. By normalizing an intrinsic active galactic nucleus (AGN) template to the AGN optical power (at 5100 Å), we decompose the total IR emission (LIR; 8–1000 µm) into an AGN (L_{IR, AGN}) and star-forming component (L_{IR, SF}). We find that the AGN contribution to L_{IR} increases as a function of AGN power, manifesting as a reduction of the ‘FIR bump’ in the average QSO SEDs. We note that L_{IR, SF} does not correlate with AGN power; the mean star formation rates (SFRs) of AGN host galaxies are a function of redshift only and they range from ∼6 M_{⊙} yr^{−1} at z ∼ 0 to a plateau of ≲ 200 M⊙ yr^{−1} at z ∼ 2.6. Our results indicate that the accuracy of FIR emission as a proxy for SFR decreases with increasing AGN luminosity. We show that, at any given redshift, observed trends between IR luminosity (whether monochromatic or total) and AGN power (in the optical or X-rays) can be explained by a simple model which is the sum of two components: (i) the IR emission from star formation, uncorrelated with AGN power and (ii) the IR emission from AGN, directly proportional to AGN power in the optical or X-rays.

Type: Article
Title: The star formation rates of QSOs
Open access status: An open access version is available from UCL Discovery
DOI: 10.1093/mnras/stac1359
Publisher version: https://doi.org/10.1093/mnras/stac1359
Language: English
Additional information: This version is the version of record. For information on re-use, please refer to the publisher's terms and conditions.
Keywords: galaxies: active, galaxies: high-redshift, quasars: general, galaxies: star formation, infrared: galaxies
UCL classification: UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL
URI: https://discovery-pp.ucl.ac.uk/id/eprint/10151988
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