出版社：SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要：Kinematic dipole signal originates from the motion of the Sun with respect to the CMB rest
frame. It is a remarkable signal, two orders of magnitude larger than the observed pattern of CMB
anisotropies. Therefore the dipole subtraction from the main beam is of primary importance. But
what happens to the dipole signal entering the main spillover (i.e. the most relevant far antenna
pattern feature, responsible for the bulk of the straylight effect)? We present here an analytical
and statistical study of this systematic effect for a spinning space-mission like PLANCK
