Joint Planck and WMAP CMB map reconstruction

We present a novel estimate of the cosmological microwave background (CMB) map by combining the two latest full-sky microwave surveys: WMAP nine-year and Planck PR1. The joint processing benefits from a recently introduced component separation method coined "local-generalized morphological component analysis" (LGMCA) and based on the sparse distribution of the foregrounds in the wavelet domain. The proposed estimation procedure takes advantage of the IRIS 100 mu m as an extra observation on the galactic center for enhanced dust removal. We show that this new CMB map presents several interesting aspects: i) it is a full sky map without using any inpainting or interpolating method; ii) foreground contamination is very low; iii) the Galactic center is very clean with especially low dust contamination as measured by the cross-correlation between the estimated CMB map and the IRIS 100 mu m map; and iv) it is free of thermal SZ contamination.


Published in:
Astronomy & Astrophysics, 563
Year:
2014
Publisher:
Les Ulis Cedex A, EDP Sciences
ISSN:
0004-6361
Keywords:
Laboratories:




 Record created 2014-05-19, last modified 2018-03-17


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