Journal article

A Comparison of Cosmological Parameters Determined from CMB Temperature Power Spectra from the South Pole Telescope and the &ITPlanck&IT Satellite

K Aylor, Z Hou, L Knox, KT Story, BA Benson, LE Bleem, JE Carlstrom, CL Chang, H-M Cho, R Chown, TM Crawford, AT Crites, T de Haan, MA Dobbs, WB Everett, EM George, NW Halverson, NL Harrington, GP Holder, WL Holzapfel Show all

ASTROPHYSICAL JOURNAL | IOP PUBLISHING LTD | Published : 2017

University of Melbourne Researchers

Grants

Awarded by U.S. Department of Energy


Awarded by National Science Foundation


Awarded by NSF Physics Frontier Center


Awarded by Australian Research Council Future Fellowship


Awarded by Fermi Research Alliance, LLC


Awarded by Gordon and Betty Moore Foundation grant


Awarded by Directorate For Geosciences


Awarded by Office of Polar Programs (OPP)


Funding Acknowledgements

The South Pole Telescope is supported by the National Science Foundation through grant PLR-1248097. Partial support is also provided by the NSF Physics Frontier Center grant PHY-1125897 to the Kavli Institute of Cosmological Physics at the University of Chicago, the Kavli Foundation and the Gordon and Betty Moore Foundation grant GBMF 947. B. Benson was supported by the Fermi Research Alliance, LLC under Contract No. DE-AC02-07CH11359 with the U.S. Department of Energy, Office of Science, Office of High Energy Physics. C. Reichardt acknowledges support from an Australian Research Council Future Fellowship (FT150100074). 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. Work at Argonne National Laboratory was supported under U.S. Department of Energy contract DE-AC02-06CH11357. This work used resources made available on the Jupiter cluster, a joint data-intensive computing project between the High Energy Physics Division and the Computing, Environment, and Fife Sciences (CELS) Directorate at Argonne National Laboratory. We thank G. Addison for pointing out the importance of the aberration correction.