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Linear polarized fluctuations in the cosmic microwave background
Limits on the linear and circular polarization of the CMB on small angular scales between 18 and 160 arcsec are reported. The procedures used are described, including the method used to discriminate against noise. No significant evidence of polarized fluctuations in the sky was found. (C.D.)
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Published in: | Nature (London) 1988-01, Vol.331 (6152), p.146-147 |
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Main Authors: | , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | Limits on the linear and circular polarization of the CMB on small angular scales between 18 and 160 arcsec are reported. The procedures used are described, including the method used to discriminate against noise. No significant evidence of polarized fluctuations in the sky was found. (C.D.) |
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ISSN: | 0028-0836 1476-4687 |
DOI: | 10.1038/331146a0 |