Journal article

Measurements of the Cross-spectra of the Cosmic Infrared and Microwave Backgrounds from 95 to 1200 GHz

MP Viero, CL Reichardt, BA Benson, LE Bleem, J Bock, JE Carlstrom, CL Chang, H-M Cho, TM Crawford, AT Crites, T de Haan, MA Dobbs, WB Everett, EM George, NW Halverson, NL Harrington, G Holder, WL Holzapfel, Z Hou, JD Hrubes Show all


University of Melbourne Researchers


Awarded by National Science Foundation

Awarded by NSF Physics Frontier Center

Awarded by Gordon and Betty Moore Foundation through grant GBMF

Awarded by Fermi Research Alliance, LLC

Awarded by Australian Research Council's Discovery Projects scheme

Awarded by Office of Science of the U.S. Department of Energy

Awarded by U.S. Department of Energy

Funding Acknowledgements

The South Pole Telescope program is supported by the National Science Foundation through grant 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 through grant GBMF#947 to the University of Chicago. The McGill authors acknowledge funding from the Natural Sciences and Engineering Research Council of Canada, Canadian Institute for Advanced Research, and Canada Research Chairs program. G.S. acknowledges support from the Fonds de recherche du Quebec-Nature et technologies. B.B. has been 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.R. acknowledges support from Australian Research Council's Discovery Projects scheme (DP150103208). This research used resources of the National Energy Research Scientific Computing Center, which is supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. 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.SPIRE has been developed by a consortium of institutes led by Cardiff Univ. (UK) and including Univ. Lethbridge (Canada); NAOC (China); CEA, LAM (France); IFSI, Univ. Padua (Italy); IAC (Spain); Stockholm Observatory (Sweden); Imperial College London, RAL, UCL-MSSL, UKATC, Univ. Sussex (UK); and Caltech, JPL, NHSC, Univ. Colorado (USA). This development has been supported by national funding agencies: CSA (Canada); NAOC (China); CEA, CNES, CNRS (France); ASI (Italy); MCINN (Spain); SNSB (Sweden); STFC, UKSA (UK); and NASA (USA). SPIRE maps were observed as part of the OT1_ jcarls01_3 program, and made from the following OBSIDS: 1342232364-5, 1342245412-4, 1342245430-2, 1342245510-2, and 1342245547.Argonne National Laboratory work was supported under U.S. Department of Energy contract DE-AC02-06CH11357.