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- W3100991755 abstract "We report upper limits on the polarization of the cosmic microwave background radiation (CMBR) as measured with the Cosmic Background Imager (CBI), a 13 element interferometer that operates in the 26-36 GHz band and is sited on Llano de Chajnantor in northern Chile. The array consists of 90 cm Cassegrain antennas mounted on a steerable platform that can be rotated about the optical axis to facilitate polarization observations. The CBI employs single-mode circularly polarized receivers, and it samples multipoles from l ~ 400 to l ~ 3500. The polarization data were calibrated on 3C 279 and Taurus A. The polarization observations consist of 278 hr of data on two fields taken in 2000, during the first CBI observing season. A joint likelihood analysis of the two fields yields three upper limits (95% confidence limit) for = CEEl(l + 1)/2π under the assumption that ≡ 0: 49.0 μK2 (l = 603), 164 μK2 (l = 1144), and 630 μK2 (l = 2048)." @default.
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- W3100991755 date "2005-04-10" @default.
- W3100991755 modified "2023-10-16" @default.
- W3100991755 title "Limits on the Polarization of the Cosmic Microwave Background Radiation at Multipoles up tol∼ 2000" @default.
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- W3100991755 doi "https://doi.org/10.1086/428384" @default.
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