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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,

Roman-Cosmic Noon: A Legacy Spectroscopic Survey of Massive Field and Protocluster Galaxies at 2 < z < 3 Thumbnail


Authors

Rudnick, Gregory

Bahé, Yannick

Balogh, Michael

Cooper, Mike

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

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