Journal article

CMB Polarization B-mode Delensing with SPTpol and Herschel

A Manzotti, KT Story, WLK Wu, JE Austermann, JA Beall, AN Bender, BA Benson, LE Bleem, JJ Bock, JE Carlstrom, CL Chang, HC Chiang, H-M Cho, R Citron, A Conley, TM Crawford, AT Crites, T de Haan, MA Dobbs, S Dodelson Show all

ASTROPHYSICAL JOURNAL | IOP PUBLISHING LTD | Published : 2017

University of Melbourne Researchers

Grants

Awarded by National Science Foundation


Awarded by NSF Physics Frontier Center


Awarded by Gordon and Betty Moore Foundation through Grant GBMF


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


Awarded by NSF


Awarded by Fermi Research Alliance, LLC


Awarded by Australian Research Councils Future Fellowship


Awarded by Direct For Mathematical & Physical Scien


Awarded by Directorate For Geosciences


Awarded by Division Of Astronomical Sciences


Awarded by Office of Polar Programs (OPP)


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. Work at Argonne National Lab is supported by UChicago Argonne, LLC, Operator of Argonne National Laboratory (Argonne). Argonne, a U.S. Department of Energy Office of Science Laboratory, is operated under Contract No. DE-AC02-06CH11357. We also acknowledge support from the Argonne Center for Nanoscale Materials. 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. This work is also supported by the U.S. Department of Energy. The CU Boulder group acknowledges support from NSF AST-0956135. BB is supported by the Fermi Research Alliance, LLC under Contract No. De-AC02-07CH11359 with the U.S. Department of Energy. C.R. acknowledges support from a Australian Research Councils Future Fellowship (FT150100074). W.L.K.W. is grateful for support from the Croucher Foundation and hospitality of Stanford University. J.W.H. is supported by the National Science Foundation under Award No. AST-1402161. The data analysis pipeline uses the scientific python stack (Jones et al. 2001; Hunter 2007; van der Walt et al. 2011) and the HDF5 file format (The HDF Group 1997). The authors acknowledge useful discussions with Blake Sherwin and Toshiya Namikawa and use of code first written by Duncan Hanson.