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E-B component separation in CMB polarization and fast simulations of CMB maps.

25 March 2015

Time: 4:30pm
Venue: G. O. Jones 516
The London Relativity and Cosmology Seminar
Dmitry Novikov (Astro Space Centre of Lebedev Physical Institute, Moscow)

A new efficient way of E and B components separation for incomplete sky coverage is presented. It is shown how to simulate full sky maps using N^2*Log(N) algorithm.

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