We describe a Two Channel Correlation Polarimeter built by the Milan Radio Group for searching polarization of the Cosmic Microwave Background. The system sensitivity is sufficient to detect linearly polarized signals or set firm upper limits at levels of few μK. The program of observations and some preliminary results are presented. © 1999 Elsevier Science B.V. All rights reserved.
Sironi, G. (1999). Polarization of the Cosmic Microwave Background: The Milan Polarimeter Experiment. NEW ASTRONOMY REVIEWS, 43(2-4), 263-269 [10.1016/S1387-6473(99)00019-6].
Polarization of the Cosmic Microwave Background: The Milan Polarimeter Experiment
SIRONI, GIORGIO
1999
Abstract
We describe a Two Channel Correlation Polarimeter built by the Milan Radio Group for searching polarization of the Cosmic Microwave Background. The system sensitivity is sufficient to detect linearly polarized signals or set firm upper limits at levels of few μK. The program of observations and some preliminary results are presented. © 1999 Elsevier Science B.V. All rights reserved.File in questo prodotto:
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