Journal article
STAR-FORMING BRIGHTEST CLUSTER GALAXIES AT 0.25 < z < 1.25: A TRANSITIONING FUEL SUPPLY
M McDonald, B Stalder, M Bayliss, SW Allen, DE Applegate, MLN Ashby, M Bautz, BA Benson, LE Bleem, M Brodwin, JE Carlstrom, I Chiu, S Desai, AH Gonzalez, J Hlavacek-Larrondo, WL Holzapfel, DP Marrone, ED Miller, CL Reichardt, BR Saliwanchik Show all
ASTROPHYSICAL JOURNAL | IOP PUBLISHING LTD | Published : 2016
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Grants
Awarded by NASA
Awarded by Hubble Fellowship grant - Space Telescope Science Institute
Awarded by National Science Foundation
Awarded by NSF Physics Frontier Center grant
Awarded by NSF
Awarded by U.S. Department of Energy
Awarded by Australian Research Councils Discovery Projects scheme
Awarded by German Federal Ministry of Economics and Technology (BMWi) through DLR
Awarded by Directorate For Geosciences
Awarded by Office of Polar Programs (OPP)
Funding Acknowledgements
We thank Mark Voit and John ZuHone for helpful conversations. M.M. acknowledges support by NASA through contracts HST-GO-13456.002A (Hubble) and GO4-15122A (Chandra), and 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 grants ANT-0638937 and PLR-1248097. 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. Galaxy cluster research at Harvard is supported by NSF grant AST-1009012 and at SAO 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. Argonne National Laboratory's work was supported under U.S. Department of Energy contract DE-AC02-06CH11357. This work is based in part on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. J.E.C. acknowledges support from National Science Foundation grants PLR-1248097 and PHY-1125897. C.R. acknowledges support from the University of Melbourne and from the Australian Research Councils Discovery Projects scheme (DP150103208). D.A. and T.S. acknowledge support from the German Federal Ministry of Economics and Technology (BMWi) provided through DLR under projects 50 OR 1210, 50 OR 1308, and 50 OR 1407.