Journal article

Galaxy Clusters Selected via the Sunyaev-Zel'dovich Effect in the SPTpol 100-square-degree Survey

N Huang, LE Bleem, B Stalder, PAR Ade, SW Allen, AJ Anderson, JE Austermann, JS Avva, JA Beall, AN Bender, BA Benson, F Bianchini, S Bocquet, M Brodwin, JE Carlstrom, CL Chang, HC Chiang, R Citron, C Corbett Moran, TM Crawford Show all

The Astronomical Journal | IOP PUBLISHING LTD | Published : 2020

University of Melbourne Researchers

Grants

Awarded by National Science Foundation


Awarded by NSF Physics Frontier Center


Awarded by Gordon and Betty Moore Foundation


Awarded by U.S. Department of Energy


Awarded by National Science Foundation Graduate Research Fellowship


Awarded by Argonne, a U.S. Department of Energy Office of Science Laboratory


Awarded by Fermi Research Alliance LLC


Awarded by NSF


Awarded by National Aeronautics and Space Administration (NASA)


Awarded by ERC-StG "ClustersXCosmo"


Awarded by FARE-MIUR grant "ClustersXEuclid"


Awarded by Australian Research Council


Funding Acknowledgements

This work was performed in the context of the South Pole Telescope scientific program. SPT is supported by the National Science Foundation through grants PLR-1248097 and 1852617. 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, and the Kavli Foundation and the Gordon and Betty Moore Foundation grant GBMF 947 to the University of Chicago. This work is also supported by the U.S. Department of Energy. This material is based upon work supported by the National Science Foundation Graduate Research Fellowship under grant No. DGE 1752814. Argonne National Laboratory's work was supported by the U.S. Department of Energy, Office of High Energy Physics. Argonne, a U.S. Department of Energy Office of Science Laboratory, is operated by UChicago Argonne LLC under contract no. DE-AC02-06CH11357. We also acknowledge support from the Argonne Center for Nanoscale Materials. B.B. is supported by the Fermi Research Alliance LLC under contract No. De-AC02-07CH11359 with the U.S. Department of Energy. The CU Boulder group acknowledges support from NSF AST-0956135. The McGill authors acknowledge funding from the Natural Sciences and Engineering Research Council of Canada, Canadian Institute for Advanced Research, and the Fonds de Recherche du Quebec Nature et Technologies. The UCLA authors acknowledge support from NSF AST-1716965 and CSSI-1835865. The Stanford/SLAC group acknowledges support from the U.S. Department of Energy under contract number DE-AC0276SF00515, and from the National Aeronautics and Space Administration (NASA) under grant No. NNX15AE12G, issued through the ROSES 2014 Astrophysics Data Analysis Program. A.S. is supported by the ERC-StG "ClustersXCosmo" grant agreement 71676, and by the FARE-MIUR grant "ClustersXEuclid" R165SBKTMA. The Melbourne group acknowledges support from the Australian Research Council's Discovery Projects scheme (DP150103208). PISCO observations are supported by NSF AST-1814719.