Rudnick, Gregory
Roman-Cosmic Noon: A Legacy Spectroscopic Survey of Massive Field and Protocluster Galaxies at 2 < z < 3
Gregory, Rudnick,; Yannick, Bahé,; Michael, Balogh,; Mike, Cooper,; Nina, Hatch,; Benedetta, Vulcani,; Gillian, Wilson,; Gianluca, Castignani,; Pierluigi, Cerulo,; Lucia, Gabriella, De; Ricardo, DeMarco,; Benjamin, Forrest,; Pascale, Jablonka,
Authors
Bahé, Yannick
Balogh, Michael
Cooper, Mike
Professor NINA HATCH nina.hatch@nottingham.ac.uk
PROFESSOR OF ASTRONOMY
Vulcani, Benedetta
Wilson, Gillian
Castignani, Gianluca
Cerulo, Pierluigi
De Lucia, Gabriella
DeMarco, Ricardo
Forrest, Benjamin
Jablonka, Pascale
Abstract
Protoclusters are the densest regions in the distant universe (z>2) and are the progenitors of massive galaxy clusters (Mhalo>1014M⊙) in the local universe. They undoubtedly play a key role in early massive galaxy evolution and they may host the earliest sites of galaxy quenching or even induce extreme states of star formation. Studying protoclusters therefore not only gives us a window into distant galaxy formation but also provides an important link in our understanding of how dense structures grow over time and modify the galaxies within them. Current protocluster samples are completely unable to address these points because they are small and selected in a heterogeneous way. We propose the Roman-Cosmic Noon survey, whose centerpiece is an extremely deep (30ksec) and wide area (10 deg2) prism slitless spectroscopy survey to identify the full range of galaxy structures at 2<z<3. This survey will include 1500 uniformly selected protoclusters, their surrounding cosmic web environments, and at least 15,000 protocluster galaxies with M⋆>1010.5M⊙ across the full range of star formation histories as well as many more lower mass star-forming galaxies. The survey will also contain field galaxies to much lower masses than in the High Latitude Wide Area Survey, but over an area dwarfing any current or planned deep spectroscopy probe at z>2. With the prism spectroscopy and some modest additional imaging this survey will measure precise stellar mass functions, quenched fractions, galaxy and protocluster morphologies, stellar ages, emission-line based SFRs, and metallicities. It will have extensive legacy value well beyond the key protocluster science goals.
Citation
Gregory, R., Yannick, B., Michael, B., Mike, C., Nina, H., Benedetta, V., Gillian, W., Gianluca, C., Pierluigi, C., Lucia, Gabriella, D., Ricardo, D., Benjamin, F., & Pascale, J. (2023). Roman-Cosmic Noon: A Legacy Spectroscopic Survey of Massive Field and Protocluster Galaxies at 2 < z < 3
Working Paper Type | Working Paper |
---|---|
Online Publication Date | Jun 27, 2023 |
Publication Date | Jun 27, 2023 |
Deposit Date | Jan 2, 2025 |
Publicly Available Date | Jan 17, 2025 |
DOI | https://doi.org/10.48550/arXiv.2306.15735 |
Public URL | https://nottingham-repository.worktribe.com/output/36305131 |
Publisher URL | https://arxiv.org/abs/2306.15735 |
Files
2306.15735v1
(2.6 Mb)
PDF
Publisher Licence URL
https://creativecommons.org/licenses/by/4.0/
You might also like
From outskirts to core: the suppression and activation of radio AGN around galaxy clusters
(2024)
Journal Article
New insights into the role of AGNs in forming the cluster red sequence
(2024)
Journal Article
Intracluster light in the core of z ∼ 2 galaxy proto-clusters
(2023)
Journal Article
Downloadable Citations
About Repository@Nottingham
Administrator e-mail: discovery-access-systems@nottingham.ac.uk
This application uses the following open-source libraries:
SheetJS Community Edition
Apache License Version 2.0 (http://www.apache.org/licenses/)
PDF.js
Apache License Version 2.0 (http://www.apache.org/licenses/)
Font Awesome
SIL OFL 1.1 (http://scripts.sil.org/OFL)
MIT License (http://opensource.org/licenses/mit-license.html)
CC BY 3.0 ( http://creativecommons.org/licenses/by/3.0/)
Powered by Worktribe © 2025
Advanced Search