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• W1908203411 abstract "We present results of polarization observations at 1.4 GHz of the two fields imaged by the DASI experiment (α= 23h30m, δ=−55° and α= 00h30m, δ=−55°, respectively). Data were taken with the Australia Telescope Compact Array with 3.4-arcmin resolution and ∼0.18-mJy beam−1 sensitivity. The emission is dominated by point sources, and we do not find evidence for diffuse synchrotron radiation even after source subtraction. This allows to estimate an upper limit of the diffuse polarized emission. The extrapolation to 30 GHz suggests that the synchrotron radiation is lower than the polarized signal measured by the DASI experiment by at least two orders of magnitude. This further supports the conclusions drawn by the DASI team itself about the negligible Galactic foreground contamination in their data set, improving by a factor of ∼5 the upper limit estimated by Leitch et al." @default.
• W1908203411 created "2016-06-24" @default.
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• W1908203411 date "2006-07-17" @default.
• W1908203411 modified "2023-10-16" @default.
• W1908203411 title "1.4-GHz polarimetric observations of the two fields imaged by the DASI experiment" @default.
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• W1908203411 doi "https://doi.org/10.1111/j.1365-2966.2006.10649.x" @default.
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