Evolved galaxies in high-density environments across 2.0 ≤ z < 4.2 using the ZFOURGE surveya

Article

Hartzenberg, Georgia R., Cowley, Michael J., Hopkins, Andrew M. and Allen, Rebecca J.. 2023. "Evolved galaxies in high-density environments across 2.0 ≤ z < 4.2 using the ZFOURGE surveya." Publications of the Astronomical Society of Australia. 40. https://doi.org/10.1017/pasa.2023.42

Article Title	Evolved galaxies in high-density environments across 2.0 ≤ z < 4.2 using the ZFOURGE surveya
ERA Journal ID	40237
Article Category	Article
Authors	Hartzenberg, Georgia R., Cowley, Michael J., Hopkins, Andrew M. and Allen, Rebecca J.
Journal Title	Publications of the Astronomical Society of Australia
Journal Citation	40
Number of Pages	10
Year	2023
Publisher	Cambridge University Press
Place of Publication	Australia
ISSN	1323-3580
	1448-6083
Digital Object Identifier (DOI)	https://doi.org/10.1017/pasa.2023.42
Web Address (URL)	https://www.cambridge.org/core/journals/publications-of-the-astronomical-society-of-australia/article/evolved-galaxies-in-highdensity-environments-across-20-z-42-using-the-zfourge-survey/2F694602C97E993EA77E21FD0F6C922B
Abstract	To explore the role environment plays in influencing galaxy evolution at high redshifts, we study <![CDATA[ $2.0\leq z environments using the FourStar Galaxy Evolution (ZFOURGE) survey. Using galaxies from the COSMOS legacy field with, we use a seventh nearest neighbour density estimator to quantify galaxy environment, dividing this into bins of low-, intermediate-, and high-density. We discover new high-density environment candidates across <![CDATA[ $2.0\leq z and <![CDATA[ $3.1\leq z. We analyse the quiescent fraction, stellar mass and specific star formation rate (sSFR) of our galaxies to understand how these vary with redshift and environment. Our results reveal that, across <![CDATA[ $2.0\leq z, the high-density environments are the most significant regions, which consist of elevated quiescent fractions, massive galaxies and suppressed star formation activity. At <![CDATA[ $3.1\leq z, we find that high-density regions consist of elevated stellar masses but require more complete samples of quiescent and sSFR data to study the effects of environment in more detail at these higher redshifts. Overall, our results suggest that well-evolved, passive galaxies are already in place in high-density environments at, and that the Butcher-Oemler effect and SFR-density relation may not reverse towards higher redshifts as previously thought. © The Author(s), 2023. Published by Cambridge University Press on behalf of the Astronomical Society of Australia.
Keywords	galaxies: evolution; galaxies: high-redshif; galaxies: groups: general
ANZSRC Field of Research 2020	5199. Other physical sciences
Byline Affiliations	Queensland University of Technology
	Centre for Astrophysics
	Macquarie University
	Swinburne University of Technology

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