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(California University of Pennsylvania), C. L. Reichardt(The University of Melbourne), I. Chiu(National Cheng Kung University), 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(Chulalongkorn University), W. L. Holzapfel(University of California, Berkeley), J. J. Mohr(Astronomical Observatory), M. McDonald(University of Chicago), 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)
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