Ettore Carretti,1 Stefano Cortiglioni,1 Claudio Macculi,1 Carla Sbarra,1 Giulio Ventura,1 Jader Monari,2 Marco Poloni,2 Sergio Poppihttps://orcid.org/0000-0002-4698-2607,2 Vincenzo Natale,3 Renzo Nesti,3 Massimo Baralis,4 Oscar A. Peverini,4 Riccardo Tascone,4 Giuseppe Virone,4 Giorgio Sironi,5 Mario Zannoni6,5
1CNR-ISAF Bologna (Italy) 2CNR-IRA Bologna (Italy) 3CNR-IRA Firenze (Italy) 4CNR-IEIIT (Italy) 5Univ. degli Studi di Milano-Bicocca (Italy) 6CNR-ISAF Milano (Italy)
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The measure of the faint polarized signal of the Cosmic Microwave Background (few percent of the CMB Anisotropy) requires instruments with very low contamination from systematic effects, high stability and high sensitivity. The BaR-SPOrt experiment, in sharing with the SPOrt project on ISS, is based on analog correlation receivers with components custom designed to match all of these requirements. Here we present the architecture, the design analysis and the status of the realization of the 32 GHz receiver.
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Ettore Carretti, Stefano Cortiglioni, Claudio Macculi, Carla Sbarra, Giulio Ventura, Jader Monari, Marco Poloni, Sergio Poppi, Vincenzo Natale, Renzo Nesti, Massimo Baralis, Oscar A. Peverini, Riccardo Tascone, Giuseppe Virone, Giorgio Sironi, Mario Zannoni, "High stability and sensitivity correlation polarimeters for CMB polarization measurements," Proc. SPIE 5498, Millimeter and Submillimeter Detectors for Astronomy II, (8 October 2004); https://doi.org/10.1117/12.551408