4.6 Article

Offset balancing in pseudo-correlation radiometers for CMB measurements

Journal

ASTRONOMY & ASTROPHYSICS
Volume 410, Issue 3, Pages 1089-1100

Publisher

E D P SCIENCES
DOI: 10.1051/0004-6361:20031266

Keywords

cosmology : cosmic microwave background, observations; instrumentation : detectors; methods : analytical

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Radiometeric CMB measurements need to be highly stable and this stability is best obtained with differential receivers. The residual 1/f noise in the differential output is strongly dependent on the radiometer input offset which can be cancelled using various balancing strategies. In this paper we discuss a software method implemented in the PLANCK-LFI pseudocorrelation receivers which uses a tunable gain modulation factor, r, in the sky-load difference. Numerical simulations and experimental data show how proper tuning of the parameter r ensures a very stable differential output with knee frequencies of the order of few mHz. Various approaches to calculate r using the radiometer total power data are discussed with some examples relevant to PLANCK-LFI. Although the paper focuses on pseudo-correlation receivers and the examples are relative to PLANCK-LFI, the proposed method and its analysis is general and can be applied to a large class of differential radiometric receivers.

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