First limits on the 21 cm power spectrum during the Epoch of X-ray heating
2016
This work was supported by NSF Grants AST-0457585,
AST-0821321, AST-1105835, AST-1410719, AST-1410484, AST-
1411622, and AST-1440343, by the MIT School of Science, by
the Marble Astrophysics Fund, and by generous donations from
Jonathan Rothberg and an anonymous donor. AEW acknowledges
support from the National Science Foundation Graduate Research
Fellowship under Grant No. 1122374. AM acknowledges support
from the European Research Council (ERC) under the European
Union’s Horizon 2020 research and innovation program (grant
agreement No 638809 – AIDA). 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 Of-
fice 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 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.
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