Ryosuke Uematsu
ALMA/SCUBA-2 COSMOS Survey: Properties of X-Ray- and SED-selected Active Galactic Nuclei in Bright Submillimeter Galaxies
Uematsu, Ryosuke; Ueda, Yoshihiro; Alexander, David M.; Swinbank, A. M.; Smail, Ian; Andonie, Carolina; Chen, Chian-Chou; Dudzevičiūtė, Ugne; Ikarashi, Soh; Kohno, Kotaro; Matsuda, Yuichi; Puglisi, Annagrazia; Umehata, Hideki; Wang, Wei-Hao
Authors
Yoshihiro Ueda
Professor David Alexander d.m.alexander@durham.ac.uk
Professor
Professor Mark Swinbank a.m.swinbank@durham.ac.uk
Professor
Ian Smail ian.smail@durham.ac.uk
Emeritus Professor
Carolina Andonie
Chian-Chou Chen
Ugne Dudzeviciute ugne.dudzeviciute2@durham.ac.uk
PGR Student Doctor of Philosophy
Soh Ikarashi
Kotaro Kohno
Yuichi Matsuda
Dr Annagrazia Puglisi annagrazia.puglisi@durham.ac.uk
Academic Visitor
Hideki Umehata
Wei-Hao Wang
Abstract
We investigate the properties of active galactic nuclei (AGNs) in the brightest submillimeter galaxies (SMGs) in the COSMOS field. We utilize the bright sample of the ALMA/SCUBA-2 COSMOS Survey (AS2COSMOS), which consists of 260 SMGs with S870 μm = 0.7–19.2 mJy at z = 0–6. We perform optical to millimeter spectral energy distribution (SED) modeling for the whole sample. We identify 24 AGN-host galaxies from the SEDs. Supplemented by 23 X-ray-detected AGNs (X-ray AGNs), we construct an overall sample of 40 AGN-host galaxies. The X-ray luminosity upper bounds indicate that the X-ray-undetected SED-identified AGNs are likely to be nearly Compton thick or have unusually suppressed X-ray emission. From visual classification, we identify 25−5+6 % of the SMGs without AGNs as major merger candidates. This fraction is almost consistent with the general galaxy population at z ∼ 2, suggesting that major mergers are not necessarily required for the enhanced star formation in SMGs. We also identify 47−15+16 % of the AGN hosts as major merger candidates, which is about twice as high as that in the SMGs without AGNs. This suggests that major mergers play a key role in triggering AGN activity in bright SMGs.
Citation
Uematsu, R., Ueda, Y., Alexander, D. M., Swinbank, A. M., Smail, I., Andonie, C., Chen, C.-C., Dudzevičiūtė, U., Ikarashi, S., Kohno, K., Matsuda, Y., Puglisi, A., Umehata, H., & Wang, W.-H. (2025). ALMA/SCUBA-2 COSMOS Survey: Properties of X-Ray- and SED-selected Active Galactic Nuclei in Bright Submillimeter Galaxies. The Astrophysical Journal, 979(2), Article 168. https://doi.org/10.3847/1538-4357/ad9f3b
Journal Article Type | Article |
---|---|
Acceptance Date | Dec 12, 2024 |
Online Publication Date | Jan 24, 2025 |
Publication Date | Feb 1, 2025 |
Deposit Date | Feb 7, 2025 |
Publicly Available Date | Feb 7, 2025 |
Journal | The Astrophysical Journal |
Electronic ISSN | 1538-4357 |
Peer Reviewed | Peer Reviewed |
Volume | 979 |
Issue | 2 |
Article Number | 168 |
DOI | https://doi.org/10.3847/1538-4357/ad9f3b |
Keywords | X-ray active galactic nuclei, Submillimeter astronomy, Active galaxies, High-redshift galaxies |
Public URL | https://durham-repository.worktribe.com/output/3351851 |
Files
Published Journal Article
(4.8 Mb)
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Publisher Licence URL
http://creativecommons.org/licenses/by/4.0/
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