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

University of Melbourne Researchers

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.