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Title: Galaxy populations in massive galaxy clusters to $$z$$ = 1.1: Color distribution, concentration, halo occupation number and red sequence fraction

Journal Article · · Monthly Notices of the Royal Astronomical Society
DOI:https://doi.org/10.1093/mnras/stx175· OSTI ID:1352814
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  1. Ludwig-Maximilians-Univ., Munich (Germany); Excellence Cluster Universe, Garching (Germany)
  2. Ludwig-Maximilians-Univ., Munich (Germany); Excellence Cluster Universe, Garching (Germany); Max Planck Institute for Extraterrestrial Physics, Garching (Germany)
  3. Ludwig-Maximilians-Univ., Munich (Germany); Cerro Tololo Inter-American Observatory, La Serena (Chile)
  4. Cerro Tololo Inter-American Observatory, La Serena (Chile)
  5. Univ. College London, London (United Kingdom); Rhodes Univ., Grahamstown (South Africa)
  6. Colby College, Waterville, ME (United States); Harvard Univ., Cambridge, MA (United States)
  7. Univ. College London, London (United Kingdom); Institut d'Astrophysique de Paris, Paris (France); Sorbonne Univ., Paris (France)
  8. Carnegie Observatories, Pasadena, CA (United States)
  9. Institut d'Astrophysique de Paris, Paris (France); Sorbonne Univ., Paris (France)
  10. Univ. College London, London (United Kingdom)
  11. Univ. of Portsmouth, Portsmouth (United Kingdom)
  12. Lab. Interinstitucional de e-Astronomia - LIneA, Rio de Janeiro (Brazil); Observatorio Nacional, Rio de Janeiro (Brazil)
  13. Univ. of Illinois, Urbana, IL (United States); National Center for Supercomputing Applications, Urbana, IL (United States)
  14. Institut de Ciencies de l'Espai, Bellaterra (Spain); The Barcelona Institute of Science and Technology, Bellaterra (Barcelona) (Spain)
  15. Univ. of Portsmouth, Portsmouth (United Kingdom); Univ. of Southampton, Southampton (United Kingdom)
  16. Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
  17. Univ. of Pennsylvania, Philadelphia, PA (United States); California Inst. of Technology (CalTech), Pasadena, CA (United States)
  18. Univ. of Michigan, Ann Arbor, MI (United States)
  19. Lab. Interinstitucional de e-Astronomia - LIneA, Rio de Janeiro (Brazil)
  20. Institut de Ciencies de l'Espai, Bellaterra (Spain)
  21. Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Univ. of Chicago, Chicago, IL (United States)
  22. Univ. of Florida, Gainesville, FL (United States)
  23. Stanford Univ., Stanford, CA (United States); SLAC National Accelerator Lab., Menlo Park, CA (United States)
  24. The Ohio State Univ., Columbus, OH (United States)
  25. Univ. de Montreal, Montreal, QC (Canada)
  26. Univ. of Pennsylvania, Philadelphia, PA (United States)
  27. Texas A & M Univ., College Station, TX (United States)
  28. Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States)
  29. Princeton Univ., Princeton, NJ (United States)
  30. The Barcelona Institute of Science and Technology, Bellaterra (Barcelona) (Spain); Institucio Catalana de Recerca i Estudis Avancats, Barcelona (Spain)
  31. California Inst. of Technology (CalTech), Pasadena, CA (United States)
  32. Univ. of Melbourne, Parkville, VIC (Australia)
  33. Univ. of Sussex, Brighton (United Kingdom)
  34. Univ. of Arizona, Tucson, AZ (United States)
  35. Centro de Investigaciones Energeticas, Madrid (Spain)
  36. Lab. Interinstitucional de e-Astronomia - LIneA, Rio de Janeiro (Brazil); Instituto de Fisica, Porto Alegre (Brazil)
  37. Univ. of Hawaii at Manoa, Honolulu, HI (United States); Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
  38. Univ. of California, Davis, CA (United States)
  39. National Center for Supercomputing Applications, Urbana, IL (United States)
  40. Argonne National Lab. (ANL), Lemont, IL (United States)
+ Show Author Affiliations

Research Organization:
Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States); SLAC National Accelerator Lab., Menlo Park, CA (United States); Argonne National Lab. (ANL), Argonne, IL (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP)
Contributing Organization:
DES Collaboration
Grant/Contract Number:
AC05-00OR22725; AC02-76SF00515; AC02-07CH11359
OSTI ID:
1352814
Alternate ID(s):
OSTI ID: 1360951; OSTI ID: 1366530
Report Number(s):
FERMILAB-PUB-16-021-AE; KJ0402000; KJ0503000; ERKJ311; ERKJEPM; TRN: US1700947
Journal Information:
Monthly Notices of the Royal Astronomical Society, Vol. 467, Issue 4; ISSN 0035-8711
Publisher:
Royal Astronomical SocietyCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 40 works
Citation information provided by
Web of Science

Cited By (10)

Galaxies in X-ray selected clusters and groups in Dark Energy Survey data – II. Hierarchical Bayesian modelling of the red-sequence galaxy luminosity function journal June 2019
The High-redshift Clusters Occupied by Bent Radio AGN (COBRA) Survey: The Spitzer Catalog journal July 2017
The Evolution of the Quenching of Star Formation in Cluster Galaxies since z ∼ 1 journal May 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
The High-redshift Clusters Occupied by Bent Radio AGN (COBRA) Survey: Follow-up Optical Imaging journal December 2019
Dark Energy Survey Year 1 Results: The Photometric Data Set for Cosmology journal April 2018
Dark Energy Survey Year 1 Results: Photometric Data Set for Cosmology text January 2018
Dark Energy Survey Year 1 Results: Photometric Data Set for Cosmology text January 2017
Galaxies in X-ray Selected Clusters and Groups in Dark Energy Survey Data II: Hierarchical Bayesian Modeling of the Red-Sequence Galaxy Luminosity Function preprint January 2017
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

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79 ASTRONOMY AND ASTROPHYSICS
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galaxies: clusters: individual
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galaxies: formation
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