Some sources of systematic errors on CMB polarized measurements with bolometers
arXiv:astro-ph/0112488 · doi:10.1063/1.1471849
Abstract
Some sources of systematic errors, specific to polarized CMB measurements using bolometers, are examined. Although the evaluations we show have been made in the context of the Planck mission (and more specifically the Planck HFI), many of our conclusions are valid for other experiments as well.
Contribution to the International workshop "Background Polarized Emission from Radio to Microwave Wavelengths" October 9-12, 2001, Bologna, Italy
Cited by in corpus (7)
- Measuring the tensor to scalar ratio from CMB B-modes in presence of foregrounds
- Beam mismatch effects in Cosmic Microwave Background polarization measurements
- Antenna Instrumental Polarization and its Effects on E- and B-Modes for CMBP Observations
- Exploring cosmic origins with CORE: mitigation of systematic effects
- Systematic effects in the measurement of polarization by the PLANCK telescope
- Systematic error mitigation for the PIXIE Fourier transform spectrometer
- Effects of Thermal Fluctuations in the SPOrt Experiment