4.7 Article

THE MASSIVE AND DISTANT CLUSTERS OF WISE SURVEY. III. SUNYAEV-ZEL'DOVICH MASSES OF GALAXY CLUSTERS AT z ∼ 1

期刊

ASTROPHYSICAL JOURNAL
卷 806, 期 1, 页码 -

出版社

IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/806/1/26

关键词

cosmology: observations; galaxies: clusters: general; galaxies: clusters: intracluster medium; galaxies: high-redshift; infrared: galaxies

资金

  1. Gordon and Betty Moore Foundation
  2. Kenneth T. and Eileen L. Norris Foundation
  3. James S. McDonnell Foundation
  4. Associates of the California Institute of Technology
  5. University of Chicago
  6. state of California
  7. state of Illinois
  8. state of Maryland
  9. National Science Foundation
  10. CARMA partner universities
  11. NSF [AST-1140019]
  12. National Aeronautics and Space Administration
  13. NASA Astrophysics Data Analysis Program (ADAP) [NNX12AE15G]
  14. NASA Keck PI Data Award
  15. W. M. Keck Foundation
  16. [PHY-0114422]
  17. [GN-2013A-Q-44]
  18. [GN-2013B-Q-8]
  19. Direct For Mathematical & Physical Scien
  20. Division Of Physics [1125897] Funding Source: National Science Foundation
  21. Division Of Astronomical Sciences
  22. Direct For Mathematical & Physical Scien [1140019, 1139950] Funding Source: National Science Foundation
  23. Division Of Astronomical Sciences
  24. Direct For Mathematical & Physical Scien [1140031, 1140063, 1139998] Funding Source: National Science Foundation

向作者/读者索取更多资源

We present CARMA 30 GHz Sunyaev-Zel'dovich (SZ) observations of five high-redshift (z greater than or similar to 1), infrared-selected galaxy clusters discovered as part of the all-sky Massive and Distant Clusters of WISE Survey (MaDCoWS). The SZ decrements measured toward these clusters demonstrate that the MaDCoWS selection is discovering evolved, massive galaxy clusters with hot intracluster gas. Using the SZ scaling relation calibrated with South Pole Telescope clusters at similar masses and redshifts, we find these MaDCoWS clusters have masses in the range M-200 approximate to 2-6 x 10(14) M-circle dot. Three of these are among the most massive clusters found to date at z greater than or similar to 1, demonstrating that MaDCoWS is sensitive to the most massive clusters to at least z = 1.3. The added depth of the AllWISE data release will allow all-sky infrared cluster detection to z approximate to 1.5 and beyond.

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