Journal article
THE GROWTH OF COOL CORES AND EVOLUTION OF COOLING PROPERTIES IN A SAMPLE OF 83 GALAXY CLUSTERS AT 0.3 < z < 1.2 SELECTED FROM THE SPT-SZ SURVEY
M McDonald, BA Benson, A Vikhlinin, B Stalder, LE Bleem, T de Haan, HW Lin, KA Aird, MLN Ashby, MW Bautz, M Bayliss, S Bocquet, M Brodwin, JE Carlstrom, CL Chang, HM Cho, A Clocchiatti, TM Crawford, AT Crites, S Desai Show all
Astrophysical Journal | IOP PUBLISHING LTD | Published : 2013
Grants
Awarded by NASA
Awarded by Association of Universities for Research in Astronomy, Inc., for NASA
Awarded by National Science Foundation
Awarded by NSF Physics Frontier Center
Awarded by NSF
Awarded by U.S. Department of Energy
Awarded by Direct For Mathematical & Physical Scien
Awarded by Directorate For Geosciences
Awarded by Division Of Astronomical Sciences
Awarded by Office of Polar Programs (OPP)
Funding Acknowledgements
M.M. acknowledges 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. The South Pole Telescope program is supported by the National Science Foundation through grant ANT-0638937. 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 Nos. 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. Galaxy cluster research at Harvard is supported by NSF grant AST-1009012 and at SAO in part by NSF grants AST-1009649 and MRI-0723073. Argonne National Laboratory's work was supported under U.S. Department of Energy contract DE-AC02-06CH11357.