Polarisation modulators are necessary for present and next generations of CMB polarisation experiments. Because of the very faint B-mode signal expected, these instruments have not only to be extremely sensitive but also to have low and well-characterised systematic effects. The beam RF characterisation in the W-band (75-110 GHz) of two polarimeter pixels using the same corrugated horn has been performed using two different modulators: a waveguide rotator modulator and a quasi-optical half-wave plate. Co- and cross-polarisation beam measurements are presented together with the systematic effects introduced by both modulators. © 2012 SPIE.

Experimental performance comparison of two polarimeter techniques for CMB applications / Maffei, B.; Pisano, G.; Ng, M. W.; Haynes, V. C.. - 8452:(2012). (Intervento presentato al convegno Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VI tenutosi a Amsterdam, nld) [10.1117/12.926911].

Experimental performance comparison of two polarimeter techniques for CMB applications

Pisano G.;
2012

Abstract

Polarisation modulators are necessary for present and next generations of CMB polarisation experiments. Because of the very faint B-mode signal expected, these instruments have not only to be extremely sensitive but also to have low and well-characterised systematic effects. The beam RF characterisation in the W-band (75-110 GHz) of two polarimeter pixels using the same corrugated horn has been performed using two different modulators: a waveguide rotator modulator and a quasi-optical half-wave plate. Co- and cross-polarisation beam measurements are presented together with the systematic effects introduced by both modulators. © 2012 SPIE.
2012
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VI
CMB instrumentation; Mm-wave components; RF characterisation
04 Pubblicazione in atti di convegno::04b Atto di convegno in volume
Experimental performance comparison of two polarimeter techniques for CMB applications / Maffei, B.; Pisano, G.; Ng, M. W.; Haynes, V. C.. - 8452:(2012). (Intervento presentato al convegno Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VI tenutosi a Amsterdam, nld) [10.1117/12.926911].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/1585648
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