Journal article

CHIPS: THE COSMOLOGICAL H I POWER SPECTRUM ESTIMATOR

CM Trott, B Pindor, P Procopio, RB Wayth, DA Mitchell, B McKinley, SJ Tingay, N Barry, AP Beardsley, G Bernardi, Judd D Bowman, F Briggs, RJ Cappallo, P Carroll, A de Oliveira-Costa, Joshua S Dillon, A Ewall-Wice, L Feng, LJ Greenhill, BJ Hazelton Show all

The Astrophysical Journal | IOP PUBLISHING LTD | Published : 2016

Grants

Awarded by Australian Research Council


Awarded by U.S. National Science Foundation


Awarded by Australian Research Council (LIEF)


Awarded by U.S. Air Force Office of Scientific Research


Awarded by Centre for All-sky Astrophysics (an Australian Research Council Centre of Excellence)


Awarded by Victoria University of Wellington from the New Zealand Ministry of Economic Development


Awarded by Victoria University of Wellington from the IBM


Awarded by Direct For Mathematical & Physical Scien


Awarded by Division Of Astronomical Sciences


Funding Acknowledgements

We thank the referee for a very thorough reading of the manuscript. and many excellent suggestions to improve its clarity. This research was supported under Australian Research Council's Discovery Early Career Researcher funding scheme (project number DE140100316). This scientific work makes use of the Murchison Radio-astronomy Observatory, operated by CSIRO. We acknowledge the Wajarri Yamatji people as the traditional owners of the Observatory site. Support for the MWA comes from the U.S. National Science Foundation (grants AST-0457585, PHY-0835713, CAREER-0847753, and AST-0908884), the Australian Research Council (LIEF grants LE0775621 and LE0882938), the U.S. Air Force Office of Scientific Research (grant FA9550-0510247), and the Centre for All-sky Astrophysics (an Australian Research Council Centre of Excellence funded by grant CE110001020). Support is also provided by the Smithsonian Astrophysical Observatory, the MIT School of Science, the Raman Research Institute, the Australian National University, and the Victoria University of Wellington (via grant MED-E1799 from the New Zealand Ministry of Economic Development and an IBM Shared University Research Grant). The Australian Federal Government provides additional support via the Commonwealth Scientific and Industrial Research Organisation (CSIRO), National Collaborative Research Infrastructure Strategy, Education Investment Fund, and the Australia India Strategic Research Fund, and Astronomy Australia Limited, under contract to Curtin University. This work was supported by resources provided by the Pawsey Supercomputing Centre with funding from the Australian Government and the Government of Western Australia. This work was supported by resources awarded under Astronomy Australia Ltds merit allocation scheme on the gSTAR national facility at Swinburne University of Technology. gSTAR is funded by Swinburne and the Australian Governments Education Investment Fund. We acknowledge the iVEC Petabyte Data Store, the Initiative in Innovative Computing and the CUDA Center for Excellence sponsored by NVIDIA at Harvard University, and the International Centre for Radio Astronomy Research (ICRAR), a Joint Venture of Curtin University and The University of Western Australia, funded by the Western Australian State Government.