Symeonidis, M;
(2021)
On the intrinsic AGN emission in the far-infrared/sub-mm.
Monthly Notices of the Royal Astronomical Society
, 509
(3)
pp. 3209-3217.
10.1093/mnras/stab3037.
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Abstract
Far-infrared (far-IR)/sub-mm emission linked to AGN-heated dust has been a topic of contention for many years. Results have been diverse and various views have been presented. The empirical AGN SED derived by Symeonidis et al. (2016, hereafter S16) has more far-IR/sub-mm emission than other SEDs in the literature, and thus it is contested by other works which argue that its luminosity in that part of the spectrum is overestimated. Here, I investigate this topic and the concerns raised over the S16 AGN SED. I also examine the differences between the S16 AGN SED and other commonly used empirical AGN SEDs. My findings show that the reasons proposed by other works as to why the S16 AGN SED is not a reasonable representation of AGN emission in the far-IR/sub-mm, do not hold.
| Type: | Article |
|---|---|
| Title: | On the intrinsic AGN emission in the far-infrared/sub-mm |
| Open access status: | An open access version is available from UCL Discovery |
| DOI: | 10.1093/mnras/stab3037 |
| Publisher version: | https://doi.org/10.1093/mnras/stab3037 |
| Language: | English |
| Additional information: | This version is the author accepted manuscript. For information on re-use, please refer to the publisher's terms and conditions. |
| Keywords: | galaxies: active, quasars: general, infrared: galaxies, infrared: general |
| UCL classification: | UCL UCL > Provost and Vice Provost Offices > UCL BEAMS 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 |
| URI: | https://discovery-pp.ucl.ac.uk/id/eprint/10137552 |
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