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Published July 2013 | Submitted + Published
Journal Article Open

A simulation-calibrated limit on the H i power spectrum from the GMRT Epoch of Reionization experiment

Abstract

The Giant Metrewave Radio Telescope Epoch of Reionization experiment is an ongoing effort to measure the power spectrum from neutral hydrogen at high redshift. We have previously reported an upper limit of (70 mK)^2 at wavenumbers of k ≈ 0.65 h Mpc^(−1) using a basic piecewise-linear foreground subtraction. In this paper, we explore the use of a singular value decomposition to remove foregrounds with fewer assumptions about the foreground structure. Using this method, we also quantify, for the first time, the signal loss due to the foreground filter and present new power spectra adjusted for this loss, providing a revised measurement of a 2σ upper limit at (248 mK)^2 for k = 0.50 h Mpc^(−1). While this revised limit is larger than previously reported, we believe it to be more robust and still represents the best current constraint on reionization at z ≈ 8.6.

Additional Information

© 2013 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. Accepted 2013 April 29. Received 2013 April 24; in original form 2013 January 24. First published online: May 27, 2013. Special thanks to Eric Switzer and Kiyoshi Masui for many useful discussions during the preparation of this work. We thank the staff of the GMRT that made these observations possible. GMRT is run by the National Centre for Radio Astrophysics of the Tata Institute of Fundamental Research. The computations were performed on CITA's Sunnyvale clusters which are funded by the Canada Foundation for Innovation, the Ontario Innovation Trust and the Ontario Research Fund. The work of GP, UP and KS is supported by the Natural Science and Engineering Research Council of Canada. KB, JP and TV are supported by NSF grant AST-1009615.

Attached Files

Published - MNRAS-2013-Paciga-639-47.pdf

Submitted - 1301.5906v2.pdf

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Created:
August 22, 2023
Modified:
October 24, 2023