The polarization status of the Cosmic Microwave Background (CMB) is still undetected. The BOOMERanG payload has been reconfigured as a scanning polarimeter, and its launch is planned for 2002. The same experimental approach has been selected for Planck-HFI and other experiments. Here we discuss some issues related to this methodology, such as the level of sensitivity required, the effects of instrumental cross-polarization and its measurement, and the best scan strategy.
Scanning polarimeters for measurements of CMB polarization
NATOLI, Paolo;
2002
Abstract
The polarization status of the Cosmic Microwave Background (CMB) is still undetected. The BOOMERanG payload has been reconfigured as a scanning polarimeter, and its launch is planned for 2002. The same experimental approach has been selected for Planck-HFI and other experiments. Here we discuss some issues related to this methodology, such as the level of sensitivity required, the effects of instrumental cross-polarization and its measurement, and the best scan strategy.File in questo prodotto:
Non ci sono file associati a questo prodotto.
I documenti in SFERA sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.