Constraining the epoch of reionization with the variance statistic: simulations of the LOFAR case
Several experiments are underway to detect the cosmic redshifted 21-cm signal from neutral hydrogen from the Epoch of Reionization (EoR). Due to their very low signal-to-noise ratio, these observations aim for a statistical detection of the signal by measuring its power spectrum. We investigate the...
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Published in | arXiv.org |
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Main Authors | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format | Paper Journal Article |
Language | English |
Published |
Ithaca
Cornell University Library, arXiv.org
16.06.2014
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Subjects | |
Online Access | Get full text |
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Summary: | Several experiments are underway to detect the cosmic redshifted 21-cm signal from neutral hydrogen from the Epoch of Reionization (EoR). Due to their very low signal-to-noise ratio, these observations aim for a statistical detection of the signal by measuring its power spectrum. We investigate the extraction of the variance of the signal as a first step towards detecting and constraining the global history of the EoR. Signal variance is the integral of the signal's power spectrum, and it is expected to be measured with a high significance. We demonstrate this through results from a simulation and parameter estimation pipeline developed for the Low Frequency Array (LOFAR)-EoR experiment. We show that LOFAR should be able to detect the EoR in 600 hours of integration using the variance statistic. Additionally, the redshift (\(z_r\)) and duration (\(\Delta z\)) of reionization can be constrained assuming a parametrization. We use an EoR simulation of \(z_r = 7.68\) and \(\Delta z = 0.43\) to test the pipeline. We are able to detect the simulated signal with a significance of 4 standard deviations and extract the EoR parameters as \(z_r = 7.72^{+0.37}_{-0.18}\) and \(\Delta z = 0.53^{+0.12}_{-0.23}\) in 600 hours, assuming that systematic errors can be adequately controlled. We further show that the significance of detection and constraints on EoR parameters can be improved by measuring the cross-variance of the signal by cross-correlating consecutive redshift bins. |
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ISSN: | 2331-8422 |
DOI: | 10.48550/arxiv.1401.4172 |