The Massive and Distant Clusters of WISE Survey. VI. Stellar Mass Fractions of a Sample of High-redshift Infrared-selected Clusters

We present measurements of the stellar mass fractions (f(star)) for a sample of high-redshift (0.93 <= z <= 1.32) infrared-selected galaxy clusters from the Massive and Distant Clusters of WISE Survey (MaDCoWS) and compare them to the stellar mass fractions of Sunyaev-Zel'dovich (SZ) effe...

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Bibliographic Details
Published in:The Astrophysical Journal
Main Authors: Decker, Bandon, Brodwin, Mark, Abdulla, Zubair, Gonzalez, Anthony H., Marrone, Daniel P., O’Donnell, Christine, Stanford, S. A., Wylezalek, Dominika, Carlstrom, John E., Eisenhardt, Peter R. M., Mantz, Adam, Mo, Wenli, Moravec, Emily, Stern, Daniel, Aldering, Greg, Ashby, Matthew L. N., Boone, Kyle, Hayden, Brian, Gupta, Nikhel, McDonald, Michael A.
Other Authors: Univ Arizona, Steward Observ
Format: Article in Journal/Newspaper
Language:English
Published: IOP PUBLISHING LTD 2019
Subjects:
Online Access:http://hdl.handle.net/10150/633516
https://doi.org/10.3847/1538-4357/ab12d7
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Summary:We present measurements of the stellar mass fractions (f(star)) for a sample of high-redshift (0.93 <= z <= 1.32) infrared-selected galaxy clusters from the Massive and Distant Clusters of WISE Survey (MaDCoWS) and compare them to the stellar mass fractions of Sunyaev-Zel'dovich (SZ) effect-selected clusters in a similar mass and redshift range from the South Pole Telescope (SPT)-SZ Survey. We do not find a significant difference in mean f(star) between the two selection methods; though, we do find an unexpectedly large range in f(star) for the SZ-selected clusters. In addition, we measure the luminosity function of the MaDCoWS clusters and find m* = 19.41 +/- 0.07, similar to other studies of clusters at or near our redshift range. Finally, we present SZ detections and masses for seven MaDCoWS clusters and new spectroscopic redshifts for five MaDCoWS clusters. One of these new clusters, MOO J1521+0452 at z = 1.31, is the most distant MaDCoWS cluster confirmed to date. Gordon and Betty Moore Foundation; Kenneth T. and Eileen L. Norris Foundation; James S. McDonnell Foundation; University of Chicago; state of California; state of Illinois; state of Maryland; National Science Foundation; NSF [AST-1140019]; NASA; National Aeronautics and Space Administration; W.M. Keck Foundation; NASA [NNX12AE15GB]; National Aeronautics and Space Administration [GO6-17130X]; National Aeronautics Space Administration [NAS8-03060]; [PHY-0114422] This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.