Journal article


RJ Foley, K Andersson, G Bazin, T de Haan, J Ruel, PAR Ade, KA Aird, R Armstrong, MLN Ashby, M Bautz, BA Benson, LE Bleem, M Bonamente, M Brodwin, JE Carlstrom, CL Chang, A Clocchiatti, TM Crawford, AT Crites, S Desai Show all


University of Melbourne Researchers


Awarded by National Science Foundation

Awarded by NASA

Awarded by DFG

Awarded by Pennsylvania State University

Awarded by Basal CATA PFB

Awarded by FONDAP

Awarded by Direct For Mathematical & Physical Scien

Awarded by Division Of Astronomical Sciences

Funding Acknowledgements

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. This work is based in part on observations obtained with the Spitzer Space Telescope (PID 60099), which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. Support for this work was provided by NASA through an award issued by JPL/Caltech. Additional data were obtained with the 6.5 m Magellan Telescopes located at the Las Campanas Observatory, Chile. Support for X-ray analysis was provided by NASA through Chandra Project Numbers 12800071 and 12800088 issued by the Chandra X-ray Observatory Center, which is operated by the Smithsonian Astrophysical Observatory for and on behalf of NASA under contract NAS8-03060. Observations from VLT programs 086.A-0741 and 286.A-5021 were included in this work. We acknowledge the use of the Legacy Archive for Microwave Background Data Analysis (LAMBDA). Support for LAMBDA is provided by the NASA Office of Space Science. Galaxy cluster research at Harvard is supported by NSF grant AST-1009012. Galaxy cluster research at SAO is supported in part by NSF grants AST-1009649 and MRI-0723073. The McGill group acknowledges funding from the National Sciences and Engineering Research Council of Canada, Canada Research Chairs program, and the Canadian Institute for Advanced Research. X-ray research at the CfA is supported through NASA Contract NAS 8-03060. The Munich group acknowledges support from the Excellence Cluster Universe and the DFG research program TR33. R.J.F. is supported by a Clay Fellowship. B. A. B. is supported by a KICP Fellowship, support for M. Brodwin was provided by the W.M. Keck Foundation, M. Bautz acknowledges support from contract 2834-MIT-SAO-4018 from the Pennsylvania State University to the Massachusetts Institute of Technology. A.C. acknowledges the support of grants Basal CATA PFB 06/09 and FONDAP No. 15010003. M.D. acknowledges support from an Alfred P. Sloan Research Fellowship, W.F. and C.J. acknowledge support from the Smithsonian Institution, and B.S. acknowledges support from the Brinson Foundation.