Hostname: page-component-8448b6f56d-gtxcr Total loading time: 0 Render date: 2024-04-19T05:33:25.608Z Has data issue: false hasContentIssue false
  • English
  • Français

A systematic search for galaxy proto-cluster cores at z ∼ 2

Published online by Cambridge University Press:  29 March 2021

Makoto Ando Open the ORCID record for Makoto Ando [Opens in a new window] ,
Kazuhiro Shimasaku  and
Rieko Momose
Makoto Ando
Affiliation:
Department of Astronomy, Graduate School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan
Kazuhiro Shimasaku
Affiliation:
Department of Astronomy, Graduate School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan Research Center for the Early Universe, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan
Rieko Momose
Affiliation:
Department of Astronomy, Graduate School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

A proto-cluster core is the most massive dark matter halo (DMH) in a given proto-cluster. To reveal the galaxy formation in core regions, we search for proto-cluster cores at z ˜ 2 in ˜1.5deg2 of the COSMOS field. Using pairs of massive galaxies (log (M*/Mʘ) ≥ 11) as tracers of cores, we find 75 candidate cores. A clustering analysis and the extended Press-Schechter model show that their descendant mass at z = 0 is consistent with Fornax-like or Virgo-like clusters. Moreover, using the IllustrisTNG simulation, we confirm that pairs of massive galaxies are good tracers of DMHs massive enough to be regarded as proto-cluster cores. We then derive the stellar mass function and the quiescent fraction for member galaxies of the 75 candidate cores. We find that stellar mass assembly and quenching are accelerated as early as z ˜ 2 in proto-cluster cores.

Keywords

galaxies: clusters: generalgalaxies: high-redshiftgalaxies: formation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S359: Galaxy Evolution and Feedback across Different Environments , March 2019 , pp. 166 - 167
Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution, and reproduction in any medium, provided the original work is properly cited.
Copyright
© The Author(s), 2021. Published by Cambridge University Press on behalf of International Astronomical Union

References

Chiang, Y.-K., Overzier, R. A., Gebhardt, K., et al. 2017, ApJ, 844, L23 10.3847/2041-8213/aa7e7bCrossRefGoogle Scholar
Laigle, C., et al. 2016, ApJS, 224, 24 10.3847/0067-0049/224/2/24CrossRefGoogle Scholar
Muldrew, S. I., Hatch, N. A., Cooke, E. A., et al. 2018, MNRAS, 473, 45, 2335 10.1093/mnras/stx2454CrossRefGoogle Scholar
Nelson, D., et al. 2019, Computational Astrophysics and Cosmology, 6, 2 10.1186/s40668-019-0028-xCrossRefGoogle Scholar