Journal article

THE EVOLUTION OF THE INTRACLUSTER MEDIUM METALLICITY IN SUNYAEV ZEL'DOVICH- SELECTED GALAXY CLUSTERS AT 0 > z > 1.5

M McDonald, E Bulbul, T de Haan, ED Miller, BA Benson, LE Bleem, M Brodwin, JE Carlstrom, I Chiu, WR Forman, J Hlavacek-Larrondo, GP Garmire, N Gupta, JJ Mohr, CL Reichardt, A Saro, B Stalder, AA Stark, JD Vieira

ASTROPHYSICAL JOURNAL | IOP PUBLISHING LTD | Published : 2016

Grants

Awarded by NASA


Awarded by NASA through a Hubble Fellowship grant - Space Telescope Science Institute


Awarded by National Science Foundation


Awarded by NSF Physics Frontier Center grant


Awarded by NASA through Chandra Award


Awarded by U.S. Department of Energy


Awarded by Australian Research Council?s Discovery Projects scheme



Awarded by Directorate For Geosciences


Awarded by Office of Polar Programs (OPP)


Funding Acknowledgements

Much of this work was enabled by generous GTO contributions from Steve Murray, and was in progress at the time of his untimely death in 2015. He was a valued member of the Center for Astrophysics and a strong supporter of SPT science-he will be greatly missed by all of us. MM acknowledges support by NASA through contracts GO4-15122A and GO5-16141X (Chandra), and support by NASA through a Hubble Fellowship grant HST-HF51308.01-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS 5-26555. EB acknowledges support by NASA through contract NNX123AE77G. The South Pole Telescope program is supported by the National Science Foundation through grants ANT-0638937 and PLR-1248097. This work was partially completed at Fermilab, operated by Fermi Research Alliance, LLC under Contract No. De-AC02-07CH11359 with the United States Department of Energy. Partial support is also provided by the NSF Physics Frontier Center grant PHY-0114422 to the Kavli Institute of Cosmological Physics at the University of Chicago, the Kavli Foundation, and the Gordon and Betty Moore Foundation. Support for X-ray analysis was provided by NASA through Chandra Award Numbers 12800071, 12800088, and 13800883 issued by the Chandra X-ray Observatory Center, which is operated by the Smithsonian Astrophysical Observatory for and on behalf of NASA. Argonne National Laboratory's work was supported under the U.S. Department of Energy contract DE-AC02-06CH11357 C. R. acknowledges support from the Australian Research Council?s Discovery Projects scheme (DP150103208).