Synthesizing Stellar Populations in South Pole Telescope Galaxy Clusters. I. Ages of Quiescent Member Galaxies at 0.3 < $$\textit{z}$$ < 1.4
Abstract
Using stellar population synthesis models to infer star formation histories (SFHs), we analyze photometry and spectroscopy of a large sample of quiescent galaxies that are members of Sunyaev–Zel'dovich (SZ)-selected galaxy clusters across a wide range of redshifts. We calculate stellar masses and mass-weighted ages for 837 quiescent cluster members at 0.3 < $$\textit{z}$$ < 1.4 using rest-frame optical spectra and the Python-based Prospector framework, from 61 clusters in the SPT-GMOS Spectroscopic Survey (0.3 < $$\textit{z}$$ < 0.9) and three clusters in the SPT Hi-z cluster sample (1.25 < $$\textit{z}$$ < 1.4). We analyze spectra of subpopulations divided into bins of redshift, stellar mass, cluster mass, and velocity-radius phase-space location, as well as by creating composite spectra of quiescent member galaxies. We find that quiescent galaxies in our data set sample a diversity of SFHs, with a median formation redshift (corresponding to the lookback time from the redshift of observation to when a galaxy forms 50% of its mass, $$t_{50}$$) of $$\textit{z}$$ = 2.8 ± 0.5, which is similar to or marginally higher than that of massive quiescent field and cluster galaxy studies. We also report median age–stellar mass relations for the full sample (age of the universe at $$t_{50}$$ (Gyr) = 2.52 (±0.04)–1.66 (±0.12) log$$_{10}(M/10^{11}M_⊙$$)) and recover downsizing trends across stellar mass; we find that massive galaxies in our cluster sample form on aggregate ~0.75 Gyr earlier than lower-mass galaxies. We also find marginally steeper age–mass relations at high redshifts, and report a bigger difference in formation redshifts across stellar mass for fixed environment, relative to formation redshifts across environment for fixed stellar mass.
- Authors:
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[1];
[2];
[3];
[2];
[4];
[5];
[7];
[4];
[8];
[9];
[4];
[10];
[11];
[12];
[13];
[14]
- Univ. of Chicago, IL (United States); Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States)
- Univ. of Cincinnati, OH (United States)
- Univ. of Chicago, IL (United States)
- Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States)
- Istituto Nazionale di Astrofisica (INAF), Trieste (Italy). Osservatorio Astronomico di Trieste; Istituto Nazionale di Astrofisica (INAF), Merate (Italy). Osservatorio Astronomico di Brera
- Univ. of Chicago, IL (United States); Argonne National Lab. (ANL), Argonne, IL (United States)
- Durham Univ. (United Kingdom)
- Univ. of Missouri, Kansas City, MO (United States)
- Univ. of Melbourne, Parkville, VIC (Australia)
- Univ. of Trieste (Italy); Institute for Fundamental Physics of the Universe (IFPU), Trieste (Italy); Osservatorio Astronomico di Trieste (Italy); National Institute for Nuclear Physics, Trieste (Italy)
- Univ. of Michigan, Ann Arbor, MI (United States)
- Stanford Univ., CA (United States). Kavli Institute for Particle Astrophysics & Cosmology
- Vera C. Rubin Observatory Project Office, Tucson, AZ (United States); Harvard & Smithsonian, Cambridge, MA (United States)
- Harvard & Smithsonian, Cambridge, MA (United States)
- Publication Date:
- Research Org.:
- Argonne National Laboratory (ANL), Argonne, IL (United States)
- Sponsoring Org.:
- National Science Foundation (NSF); Gordon and Betty Moore Foundation; USDOE Office of Science (SC), High Energy Physics (HEP); Australian Research Council (ARC); European Union’s Horizon 2020; European Research Council (ERC); Ministry of Education, University and Research (MIUR)
- OSTI Identifier:
- 1958319
- Grant/Contract Number:
- AC02-06CH11357; PLR-1248097; OPP-1852617; PHY-1125897; GBMF#947; MARACAS-DLV-896778; 716762; R165SBKTMA
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal
- Additional Journal Information:
- Journal Volume: 934; Journal Issue: 2; Journal ID: ISSN 0004-637X
- Publisher:
- IOP Publishing
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; Galaxy Clusters: High-redshift galaxy clusters; galaxies: quenched galaxies; galaxy evolution: galaxy quenching; photometry: spectral energy distribution; spectroscopy: galaxy spectroscopy
Citation Formats
Khullar, Gourav, Bayliss, Matthew B., Gladders, Michael D., Kim, Keunho J., Calzadilla, Michael S., Strazzullo, Veronica, Bleem, Lindsey E., Mahler, Guillaume, McDonald, Michael, Floyd, Benjamin, Reichardt, Christian L., Ruppin, Florian, Saro, Alexandro, Sharon, Keren, Somboonpanyakul, Taweewat, Stalder, Brian, and Stark, Antony A. Synthesizing Stellar Populations in South Pole Telescope Galaxy Clusters. I. Ages of Quiescent Member Galaxies at 0.3 < $\textit{z}$ < 1.4. United States: N. p., 2022.
Web. doi:10.3847/1538-4357/ac7c0c.
Khullar, Gourav, Bayliss, Matthew B., Gladders, Michael D., Kim, Keunho J., Calzadilla, Michael S., Strazzullo, Veronica, Bleem, Lindsey E., Mahler, Guillaume, McDonald, Michael, Floyd, Benjamin, Reichardt, Christian L., Ruppin, Florian, Saro, Alexandro, Sharon, Keren, Somboonpanyakul, Taweewat, Stalder, Brian, & Stark, Antony A. Synthesizing Stellar Populations in South Pole Telescope Galaxy Clusters. I. Ages of Quiescent Member Galaxies at 0.3 < $\textit{z}$ < 1.4. United States. https://doi.org/10.3847/1538-4357/ac7c0c
Khullar, Gourav, Bayliss, Matthew B., Gladders, Michael D., Kim, Keunho J., Calzadilla, Michael S., Strazzullo, Veronica, Bleem, Lindsey E., Mahler, Guillaume, McDonald, Michael, Floyd, Benjamin, Reichardt, Christian L., Ruppin, Florian, Saro, Alexandro, Sharon, Keren, Somboonpanyakul, Taweewat, Stalder, Brian, and Stark, Antony A. Thu .
"Synthesizing Stellar Populations in South Pole Telescope Galaxy Clusters. I. Ages of Quiescent Member Galaxies at 0.3 < $\textit{z}$ < 1.4". United States. https://doi.org/10.3847/1538-4357/ac7c0c. https://www.osti.gov/servlets/purl/1958319.
@article{osti_1958319,
title = {Synthesizing Stellar Populations in South Pole Telescope Galaxy Clusters. I. Ages of Quiescent Member Galaxies at 0.3 < $\textit{z}$ < 1.4},
author = {Khullar, Gourav and Bayliss, Matthew B. and Gladders, Michael D. and Kim, Keunho J. and Calzadilla, Michael S. and Strazzullo, Veronica and Bleem, Lindsey E. and Mahler, Guillaume and McDonald, Michael and Floyd, Benjamin and Reichardt, Christian L. and Ruppin, Florian and Saro, Alexandro and Sharon, Keren and Somboonpanyakul, Taweewat and Stalder, Brian and Stark, Antony A.},
abstractNote = {Using stellar population synthesis models to infer star formation histories (SFHs), we analyze photometry and spectroscopy of a large sample of quiescent galaxies that are members of Sunyaev–Zel'dovich (SZ)-selected galaxy clusters across a wide range of redshifts. We calculate stellar masses and mass-weighted ages for 837 quiescent cluster members at 0.3 < $\textit{z}$ < 1.4 using rest-frame optical spectra and the Python-based Prospector framework, from 61 clusters in the SPT-GMOS Spectroscopic Survey (0.3 < $\textit{z}$ < 0.9) and three clusters in the SPT Hi-z cluster sample (1.25 < $\textit{z}$ < 1.4). We analyze spectra of subpopulations divided into bins of redshift, stellar mass, cluster mass, and velocity-radius phase-space location, as well as by creating composite spectra of quiescent member galaxies. We find that quiescent galaxies in our data set sample a diversity of SFHs, with a median formation redshift (corresponding to the lookback time from the redshift of observation to when a galaxy forms 50% of its mass, $t_{50}$) of $\textit{z}$ = 2.8 ± 0.5, which is similar to or marginally higher than that of massive quiescent field and cluster galaxy studies. We also report median age–stellar mass relations for the full sample (age of the universe at $t_{50}$ (Gyr) = 2.52 (±0.04)–1.66 (±0.12) log$_{10}(M/10^{11}M_⊙$)) and recover downsizing trends across stellar mass; we find that massive galaxies in our cluster sample form on aggregate ~0.75 Gyr earlier than lower-mass galaxies. We also find marginally steeper age–mass relations at high redshifts, and report a bigger difference in formation redshifts across stellar mass for fixed environment, relative to formation redshifts across environment for fixed stellar mass.},
doi = {10.3847/1538-4357/ac7c0c},
journal = {The Astrophysical Journal},
number = 2,
volume = 934,
place = {United States},
year = {Thu Aug 04 00:00:00 EDT 2022},
month = {Thu Aug 04 00:00:00 EDT 2022}
}
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