X-Ray Properties of SPT-selected Galaxy Clusters at 0.2 < z < 1.5 Observed with XMM-Newton
Esra Bulbul, I-Non Chiu, Joseph J Mohr, Michael McDonald, Bradford Benson, Mark W Bautz, Matthew Bayliss, Lindsey Bleem, Mark Brodwin, Sebastian Bocquet, Raffaella Capasso, Joerg P Dietrich, Bill Forman, Julie Hlavacek-Larrondo, WL Holzapfel, Gourav Khullar, Matthias Klein, Ralph Kraft, Eric D Miller, Christian Reichardt Show all
The Astrophysical Journal | IOP PUBLISHING LTD | Published : 2019
Awarded by DLR award
Awarded by National Science Foundation
Awarded by NSF Physics Frontier Center grant
Awarded by Gordon and Betty Moore Foundation
The authors thank the anonymous referee and David Rapetti for helpful comments on the draft. We acknowledge the support by the DFG Cluster of Excellence "Origin and Structure of the Universe," the DLR award 50 OR 1205 that supported I. Chiu during his PhD project, and the Transregio program TR33 "The Dark Universe. "The South Pole Telescope is supported by the National Science Foundation through grant PLR-1248097. Partial support is also provided by the NSF Physics Frontier Center grant PHY-1125897 to the Kavli Institute of Cosmological Physics at the University of Chicago, the Kavli Foundation, and the Gordon and Betty Moore Foundation grant GBMF 947.