Rhythm Shimakawa
New insights into the role of AGNs in forming the cluster red sequence
Shimakawa, Rhythm; Pérez-Martínez, Jose Manuel; Koyama, Yusei; Tanaka, Masayuki; Tanaka, Ichi; Kodama, Tadayuki; Hatch, Nina A.; Röttgering, Huub J.A.; Dannerbauer, Helmut; Kurk, Jaron D.
Authors
Jose Manuel Pérez-Martínez
Yusei Koyama
Masayuki Tanaka
Ichi Tanaka
Tadayuki Kodama
Professor NINA HATCH nina.hatch@nottingham.ac.uk
PROFESSOR OF ASTRONOMY
Huub J.A. Röttgering
Helmut Dannerbauer
Jaron D. Kurk
Abstract
As a considerable investment of time from various telescope facilities was dedicated toward studying the Spiderweb protocluster at z = 2.2, it so far remains one of the most extensively studied protocluster. We report here the latest results in this field, adding a new dimension to previous research on cluster formation at high redshift. Previous studies have reported a significant overdensity (δ ∼ 10) of massive Hα (+ [N ii])-emitting galaxies in 3700 comoving Mpc3. Many of these were previously considered to be dusty, actively star-forming galaxies, given their rest-frame optical and infrared features. However, this study argues that a third of them are more likely to be ‘passively evolving’ galaxies with low-luminosity active galactic nuclei (AGNs) rather than star-forming galaxies, given the multiwavelength spectral energy distribution (SED) fitting including an AGN component. For their SED-based star formation rates to be valid, bulk of their Hα + [N ii] emission should come from the central AGNs. This difference in interpretation between this work and past studies, including ours, is particularly supported by the recent deep Chandra/X-ray observation. Furthermore, we have spectroscopically confirmed a quiescent nature for one of these AGNs, with its multiple stellar absorption lines but also low-ionization emission lines. This important update provides new insights into the role of AGNs in forming the cluster red sequence observed in the present-day universe.
Citation
Shimakawa, R., Pérez-Martínez, J. M., Koyama, Y., Tanaka, M., Tanaka, I., Kodama, T., Hatch, N. A., Röttgering, H. J., Dannerbauer, H., & Kurk, J. D. (2024). New insights into the role of AGNs in forming the cluster red sequence. Monthly Notices of the Royal Astronomical Society, 528(2), 3679–3695. https://doi.org/10.1093/mnras/stae118
Journal Article Type | Article |
---|---|
Acceptance Date | Jan 10, 2024 |
Online Publication Date | Jan 11, 2024 |
Publication Date | 2024-02 |
Deposit Date | Mar 17, 2024 |
Publicly Available Date | Mar 17, 2024 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Oxford University Press |
Peer Reviewed | Peer Reviewed |
Volume | 528 |
Issue | 2 |
Pages | 3679–3695 |
DOI | https://doi.org/10.1093/mnras/stae118 |
Keywords | galaxies: clusters: individual: PKS 1138−262, galaxies: evolution, galaxies: formation, galaxies: high-redshift |
Public URL | https://nottingham-repository.worktribe.com/output/29842273 |
Publisher URL | https://academic.oup.com/mnras/article/528/2/3679/7517094 |
Files
2306.06392
(3.3 Mb)
PDF
Publisher Licence URL
https://creativecommons.org/licenses/by/4.0/
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