TY - JOUR
T1 - The Massive and Distant Clusters of WISE Survey. VI. Stellar Mass Fractions of a Sample of High-redshift Infrared-selected Clusters
AU - Decker, Bandon
AU - Brodwin, Mark
AU - Abdulla, Zubair
AU - Gonzalez, Anthony H.
AU - Marrone, Daniel P.
AU - O'Donnell, Christine
AU - Stanford, S. A.
AU - Wylezalek, Dominika
AU - Carlstrom, John E.
AU - Eisenhardt, Peter R.M.
AU - Mantz, Adam
AU - Mo, Wenli
AU - Moravec, Emily
AU - Stern, Daniel
AU - Aldering, Greg
AU - Ashby, Matthew L.N.
AU - Boone, Kyle
AU - Hayden, Brian
AU - Gupta, Nikhel
AU - McDonald, Michael A.
N1 - Publisher Copyright:
© 2019. The American Astronomical Society. All rights reserved.
PY - 2019/6/10
Y1 - 2019/6/10
N2 - We present measurements of the stellar mass fractions ( f∗) 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∗ between the two selection methods; though, we do find an unexpectedly large range in f∗ 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.
AB - We present measurements of the stellar mass fractions ( f∗) 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∗ between the two selection methods; though, we do find an unexpectedly large range in f∗ 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.
KW - cosmology: observations
KW - galaxies: clusters: general
KW - galaxies: clusters: intracluster medium
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U2 - 10.3847/1538-4357/ab12d7
DO - 10.3847/1538-4357/ab12d7
M3 - Article
AN - SCOPUS:85069486144
VL - 878
JO - Astrophysical Journal
JF - Astrophysical Journal
SN - 0004-637X
IS - 1
M1 - 72
ER -