The GMRT Epoch of Reionization experiment: a new upper limit on the neutral hydrogen power spectrum at z ≈ 8.6

Paciga, Gregory ; Chang, Tzu-Ching ; Gupta, Yashwant ; Nityanada, Rajaram ; Odegova, Julia ; Pen, Ue-Li ; Peterson4, Jeffrey B. ; Roy, Jayanta ; Sigurdson, Kris (2011) The GMRT Epoch of Reionization experiment: a new upper limit on the neutral hydrogen power spectrum at z ≈ 8.6 Monthly Notices of the Royal Astronomical Society, 413 (2). pp. 1174-1183. ISSN 0035-8711

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Official URL: http://onlinelibrary.wiley.com/doi/10.1111/j.1365-...

Related URL: http://dx.doi.org/10.1111/j.1365-2966.2011.18208.x

Abstract

We present a new upper limit to the 21-cm power spectrum during the Epoch of Reionization (EoR) which constrains reionization models with an unheated IGM. The GMRT-EoR experiment is an ongoing effort to make a statistical detection of the power spectrum of 21-cm neutral hydrogen emission at redshift z~ 9. Data from this redshift constrain models of the EoR, the end of the Dark Ages arising from the formation of the first bright UV sources, probably stars or mini-quasars. We present results from approximately 50 h of observations with the Giant Metrewave Radio Telescope in India from 2007 December. We describe radio-frequency interference (RFI) localization schemes which allow bright sources on the ground to be identified and physically removed in addition to automated flagging. Singular-value decomposition is used to remove the remaining broad-band RFI by identifying ground sources with large eigenvalues. Foregrounds are modelled using a piecewise linear filter and the power spectrum is measured using cross-correlations of foreground-subtracted images.

Item Type:Article
Source:Copyright of this article belongs to John Wiley and Sons.
Keywords:Intergalactic Medium; Cosmology: Observations; Dark Ages; Reionization; First Stars; Diffuse Radiation; Radio Lines: General
ID Code:92177
Deposited On:26 May 2012 14:03
Last Modified:26 May 2012 14:03

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