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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

ALMA/SCUBA-2 COSMOS Survey: Properties of X-Ray- and SED-selected Active Galactic Nuclei in Bright Submillimeter Galaxies Thumbnail


Authors

Ryosuke Uematsu

Yoshihiro Ueda

Profile image of Ian Smail

Ian Smail ian.smail@durham.ac.uk
Emeritus Professor

Carolina Andonie

Chian-Chou Chen

Soh Ikarashi

Kotaro Kohno

Yuichi Matsuda

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

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