Destriping Polarised data


Polarisation measurements on the Cosmological Microwave Background (CMB) will be very difficult as the expected polarisation is not expected to exceed 10% of the signal. Therefore, noises of all origins must be searched for and carefully extracted. Low frequency drifts are expected to arise from mechanic, thermal and electronic origin. If not suitably… (More)


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@inproceedings{Revenu1998DestripingPD, title={Destriping Polarised data}, author={Benoı̂t Revenu}, year={1998} }