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

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

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Author(s)
Brodwin, M.
•
Greer, C. H.
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Leitch, E. M.
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Stanford, S. A.
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Gonzalez, A. H.
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Gettings, D. P.
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Abdulla, Z.
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Carlstrom, J. E.
•
Decker, B.
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Eisenhardt, P. R.
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Date Issued
June 2015
Journal
The Astrophysical Journal
Publisher
IOP Publishing
Citation
Brodwin, M., C. H. Greer, E. M. Leitch, S. A. Stanford, A. H. Gonzalez, D. P. Gettings, Z. Abdulla, et al. “THE MASSIVE AND DISTANT CLUSTERS OF WISE SURVEY. III. SUNYAEV–ZEL’DOVICH MASSES OF GALAXY CLUSTERS AT z ~ 1.” The Astrophysical Journal 806, no. 1 (June 5, 2015): 26. © 2015 The American Astronomical Society
Version
Final published version
Abstract
We present CARMA 30 GHz Sunyaev–Zel'dovich (SZ) observations of five high-redshift (z [> over ~] 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[subscript 200] ≈ 2-6 X 10[superscript 14] M[subscript ʘ. Three of these are among the most massive clusters found to date at z [> over ~] 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 ≈ 1.5 and beyond.
MIT Department
Massachusetts Institute of Technology. Department of Physics
MIT Kavli Institute for Astrophysics and Space Research
Terms of Use
Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
Persistent DSpace Link
http://hdl.handle.net/1721.1/98312
DOI of Published Version
https://doi.org/10.1088/0004-637x/806/1/26
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