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19 April 2024
 
  » arxiv » 1502.5072

 Article overview


New Limits on Polarized Power Spectra at 126 and 164 MHz: Relevance to Epoch of Reionization Measurements
David Moore ; James E. Aguirre ; Aaron Parsons ; Zaki Ali ; Richard Bradley ; Chris Carilli ; David DeBoer ; Matthew Dexter ; Nicole Gugliucci ; Daniel Jacobs ; Pat Klima ; Adrian Liu ; David MacMahon ; Jason Manley ; Jonathan Pober ; Irina Stefan ; William Walbrugh ;
Date 17 Feb 2015
AbstractPolarized foreground emission is a potential contaminant of attempts to measure the fluctuation power spectrum of highly redshifted 21 cm H{sc i} emission from the epoch of reionization, yet observational constraints on the level of polarized emission are poor. Using the Donald C. Backer Precision Array for Probing the Epoch of Reionization (PAPER), we present the first limits on the power spectra of all four Stokes parameters in two frequency bands, centered at 126 MHz ($z=10.3$) and 164 MHz ($z=7.66$). This data comes from from a three-month observing campaign of a 32-antenna deployment, for which unpolarized power spectrum results have been reported at $z=7.7$ (Parsons et al 2014) and $7.5 < z < 10.5$ (Jacobs et al 2014). The power spectra in this paper are processed in the same way, and show no definitive detection of polarized power. The limits are sufficiently low that we are able to show that the excess unpolarized power reported in those works is not due to leakage of Faraday-rotated polarized emission. Building upon the Moore et al 2013 simulations of polarized point sources, we further argue that our upper limits and previous observations imply that the mean polarization fraction of point sources at these frequencies is $sim2 imes10^{-3}$, roughly an order of magnitude lower than that observed for point sources at 1.4 GHz.
Source arXiv, 1502.5072
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