The role of mass and environment in the build-up of the quenched galaxy population since cosmic noon

Taylor, Elizabeth; Almaini, Omar; Merrifield, Michael; Maltby, David; Wild, Vivienne; Hartley, William G.; Rowlands, Kate

Abstract

We conduct the first study of how the relative quenching probability of galaxies depends on environment over the redshift range 0.5 < z < 3, using data from the UKIDSS Ultra-Deep Survey. By constructing the stellar mass functions for quiescent and post-starburst (PSB) galaxies in high-, medium- and low-density environments to z = 3, we find an excess of quenched galaxies in dense environments out to at least z ∼ 2. Using the growth rate in the number of quenched galaxies, combined with the star-forming galaxy mass function, we calculate the probability that a given star-forming galaxy is quenched per unit time. We find a significantly higher quenching rate in dense environments (at a given stellar mass) at all redshifts. Massive galaxies (M * > 10 10.7 M ⊙) are on average 1.7 ± 0.2 times more likely to quench per Gyr in the densest third of environments compared to the sparsest third. Finally, we compare the quiescent galaxy growth rate to the rate at which galaxies pass through a PSB phase. Assuming a visibility time-scale of 500 Myr, we find that the PSB route can explain ∼ 50 per cent of the growth in the quiescent population at high stellar mass (M * > 10 10.7 M ⊙) in the redshift range 0.5 < z < 3, and potentially all of the growth at lower stellar masses.

Citation

Taylor, E., Almaini, O., Merrifield, M., Maltby, D., Wild, V., Hartley, W. G., & Rowlands, K. (2023). The role of mass and environment in the build-up of the quenched galaxy population since cosmic noon. Monthly Notices of the Royal Astronomical Society, 522(2), 2297-2306. https://doi.org/10.1093/mnras/stad1098

• Journal Article Type: Article
• Acceptance Date: Apr 5, 2023
• Online Publication Date: Apr 14, 2023
• Publication Date: 2023-06
• Deposit Date: Apr 18, 2023
• Publicly Available Date: Apr 19, 2023
• Journal: Monthly Notices of the Royal Astronomical Society
• Print ISSN: 0035-8711
• Electronic ISSN: 1365-2966
• Publisher: Oxford University Press (OUP)
• Peer Reviewed: Peer Reviewed
• Volume: 522
• Issue: 2
• Pages: 2297-2306
• DOI: https://doi.org/10.1093/mnras/stad1098
• Keywords: Galaxies: evolution, galaxies: formation, galaxies: luminosity function, mass function, galaxies: high-redshift
• Public URL: https://nottingham-repository.worktribe.com/output/19761304
• Publisher URL: https://academic.oup.com/mnras/article/522/2/2297/7120050
• Additional Information: © The Author(s) 2023. Published by Oxford University Press on behalf of Royal Astronomical Society.; This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.