X-Ray Properties of SPT-selected Galaxy Clusters at 0.2 < z < 1.5 Observed with XMM-Newton

Esra Bülbül(Center for Astrophysics Harvard & Smithsonian), Adam Stanford(University of California, Davis), S. Bocquet(Ludwig-Maximilians-Universität München), C. L. Reichardt(The University of Melbourne), I. Chiu(Institute of Astronomy and Astrophysics, Academia Sinica), Keren Sharon(University of Michigan), Gourav Khullar(University of Chicago), Eric D. Miller(Massachusetts Institute of Technology), Matthew Bayliss(University of North Carolina at Chapel Hill), T. Schrabback(Leiden University), B. A. Benson(Fermi National Accelerator Laboratory), L. E. Bleem(Argonne National Laboratory), Julie Hlavacek-Larrondo(Université de Montréal), Ralph Kraft(Center for Astrophysics Harvard & Smithsonian), B. Stalder(Large Synoptic Survey Telescope Corporation), W. L. Holzapfel(University of California, Berkeley), J. J. Mohr(Max Planck Institute for Extraterrestrial Physics), M. McDonald(Massachusetts Institute of Technology), Matthias Klein(Ludwig-Maximilians-Universität München), J. P. Dietrich(University of Bonn), M. Brodwin(University of Missouri–Kansas City), Mark W. Bautz(Massachusetts Institute of Technology), R. Capasso(Trieste Astronomical Observatory)
The Astrophysical Journal
January 20, 2019
Cited by 125


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