Journal article

SPT-CL J0205-5829: A z=1.32 EVOLVED MASSIVE GALAXY CLUSTER IN THE SOUTH POLE TELESCOPE SUNYAEV-ZEL'DOVICH EFFECT SURVEY

B Stalder, J Ruel, R Suhada, M Brodwin, KA Aird, K Andersson, R Armstrong, MLN Ashby, M Bautz, M Bayliss, G Bazin, BA Benson, LE Bleem, JE Carlstrom, CL Chang, HM Cho, A Clocchiatti, TM Crawford, AT Crites, T de Haan Show all

ASTROPHYSICAL JOURNAL | IOP PUBLISHING LTD | Published : 2013

University of Melbourne Researchers

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Awarded by National Science Foundation


Awarded by NSF Physics Frontier Center


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Awarded by NASA


Awarded by DFG


Awarded by Pennsylvania State University


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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. 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. 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 and the Blanco 4 m Telescope at Cerro Tololo Inter-American Observatories in Chile. R.J.F. is supported by a Clay Fellowship. B. A. B is supported by a KICP Fellowship, M. Bautz acknowledges support from contract 2834-MIT-SAO-4018 from the Pennsylvania State University to the Massachusetts Institute of Technology. M. D. acknowledges support from an Alfred P. Sloan Research Fellowship, W. F. and C.J. acknowledge support from the Smithsonian Institution.