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Title: Galaxy populations in the most distant SPT-SZ clusters: I. Environmental quenching in massive clusters at 1.4 ≲ z ≲ 1.7

Journal Article · · Astronomy and Astrophysics
 [1];  [1];  [2];  [3];  [4];  [5];  [1];  [4];  [6];  [7];  [8];  [9];  [10];  [11];  [7];  [12];  [13];  [14];  [15];  [16] more »;  [17];  [5];  [7];  [18];  [19];  [20];  [21];  [22] « less
  1. Ludwig-Maximilians-Univ., Munich (Germany)
  2. Ludwig-Maximilians-Univ., Munich (Germany); Max Planck Institute for Extraterrestrial Physics, Garching (Germany); Excellence Cluster Universe, Garching (Germany)
  3. Ludwig-Maximilians-Univ., Munich (Germany); INAF-Osservatorio Astronomico di Trieste, Trieste (Italy)
  4. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
  5. Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States)
  6. Univ. of Chicago, Chicago, IL (United States)
  7. Stanford Univ., Stanford, CA (United States)
  8. Univ. of California, Davis, CA (United States)
  9. Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Univ. of Chicago, Chicago, IL (United States)
  10. Argonne National Lab. (ANL), Argonne, IL (United States); Univ. of Chicago, Chicago, IL (United States)
  11. Univ. of Missouri, Kansas City, MO (United States)
  12. Ludwig-Maximilians-Univ., Munich (Germany); Excellence Cluster Universe, Garching (Germany)
  13. Academia Sinica Institute of Astronomy and Astrophysics, Taipei (Taiwan)
  14. Univ. of Florida, Gainesville, FL (United States)
  15. Ludwig-Maximilians-Univ., Munich (Germany); Excellence Cluster Universe, Garching (Germany); Univ. of Melbourne, Parkville, VIC (Australia)
  16. Univ. of Montreal, Montreal, QC (Canada)
  17. Ludwig-Maximilians-Univ., Munich (Germany); Max Planck Institute for Extraterrestrial Physics, Garching (Germany)
  18. Univ. of Colorado, Boulder, CO (United States); NASA Ames Research Center, Moffett Field, CA (United States)
  19. Univ. of Melbourne, Parkville, VIC (Australia)
  20. Argelander-Institut fur Astronomie, Bonn (Germany)
  21. Univ. of Michigan, Ann Arbor, MI (United States)
  22. LSST, Tucson, AZ (United States)
+ Show Author Affiliations

Here, we present the first results from a galaxy population study in the highest redshift galaxy clusters identified in the 2500 deg2 South Pole Telescope Sunyaev Zel’dovich effect (SPT-SZ) survey, which is sensitive to M500 ≳ 3 × 1014 M⊙ clusters from z ~ 0.2 out to the highest redshifts where such massive structures exist. The cluster selection is to first order independent of galaxy properties, making the SPT-SZ sample particularly well suited for cluster galaxy population studies. We carried out a four-band imaging campaign with the Hubble and Spitzer Space Telescopes of the five z ≳ 1.4, S/NSZE > 5 clusters, that are among the rarest most massive clusters known at this redshift. All five clusters show clear overdensities of red galaxies whose colors agree with the initial cluster redshift estimates, although one (SPT-CLJ0607–4448) shows a galaxy concentration much less prominent than the others. The highest redshift cluster in this sample, SPT-CLJ0459–4947 at z ~ 1.72, is the most distant M500 > 1014 M⊙ cluster discovered thus far through its intracluster medium, and is one of only three known clusters in this mass range at z ≳ 1.7, regardless of selection. Based on UVJ-like photometric classification of quiescent and star-forming galaxies, we find that the quiescent fraction in the cluster central regions (r/r500 < 0.7) is higher than in the field at the same redshift, with corresponding environmental quenching efficiencies typically in the range ~0.5 – 0.8 for stellar masses log(M/M⊙) > 10.85. We have explored the impact of emission from star formation on the selection of this sample, concluding that all five clusters studied here would still have been detected with S/NSZE > 5, even if they had the same quiescent fraction as measured in the field. Our results thus point towards an efficient suppression of star formation in the central regions of the most massive clusters, occurring already earlier than z ~ 1.5.

Research Organization:
Argonne National Lab. (ANL), Argonne, IL (United States)
Sponsoring Organization:
Deutsche Forschungsgemeinschaft (DFG); European Research Council (ERC); German Aerospace Center; German Federal Ministry of Education and Research (BMBF); USDOE
Grant/Contract Number:
AC02-06CH11357
OSTI ID:
1496035
Journal Information:
Astronomy and Astrophysics, Journal Name: Astronomy and Astrophysics Vol. 622; ISSN 0004-6361
Publisher:
EDP SciencesCopyright Statement
Country of Publication:
United States
Language:
English

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Cited By (13)

The dependence of AGN activity on environment in SDSS journal June 2019
Evolution of star formation rate–density relation over cosmic time in a simulated universe: the observed reversal reproduced journal August 2019
Persistence of the colour–density relation and efficient environmental quenching to z ∼ 1.4 journal September 2019
Mass calibration of the CODEX cluster sample using SPIDERS spectroscopy – I. The richness–mass relation journal March 2019
On the Origin of the Scatter in the Red Sequence: An Analysis of Four CLASH Clusters journal April 2019
Cluster Cosmology Constraints from the 2500 deg 2 SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope journal June 2019
Large Molecular Gas Reservoirs in Star-forming Cluster Galaxies journal September 2019
On the Gas Content, Star Formation Efficiency, and Environmental Quenching of Massive Galaxies in Protoclusters at z ≈ 2.0–2.5 journal December 2019
Cluster Cosmology Constraints from the 2500 deg$^2$ SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope text January 2018
On the Origin of the Scatter in the Red Sequence: An Analysis of Four CLASH Clusters text January 2019
The Dependence of AGN Activity on Environment in SDSS text January 2019
Large Molecular Gas Reservoirs in Star Forming Cluster Galaxies text January 2019
On the Gas Content, Star Formation Efficiency, and Environmental Quenching of Massive Galaxies in Proto-Clusters at z~2.0-2.5 text January 2019

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