Feb 20, 2015 · Abstract:We present foreground-reduced CMB maps derived from the full Planck data set in both temperature and polarization.
The component separation pipelines are principally designed to remove diffuse foreground emission from the CMB, so residuals from unresolved compact sources ...
Feb 5, 2015 · In this paper we consider the problem of diffuse astrophysical component separation, and process these maps within a Bayesian framework to ...
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Planck 2015 results IX. Diffuse component separation: CMB maps. Adam, R.; Ade, P. A R; Aghanim, N.; Arnaud, M.; Ashdown, M.; Aumont, J.; Baccigalupi, C ...
Authors Planck Collaboration • Adam, R. Ade, P. A. R. · Abstract We present foreground-reduced cosmic microwave background (CMB) maps derived from the full ...
Differences between the component-separated CMB temperature maps from the 2013 and the 2015 releases. The maps have been smoothed to FWHM 80\arcm\ and ...
As in 2013, four different CMB component separation algorithms are applied to these observations, providing a measure of stability with respect to algorithmic ...
Dec 31, 2015 · Planck 2015 results IX. Diffuse component separation: CMB maps. Authors. Eduardo Battaner López. Publication date: 31 December 2015. Publisher ...
Feb 24, 2015 · We present foreground-reduced CMB maps derived from the full Planck data set in both temperature and polarization.
Since we are studying large scale structures, the foreground contamination may be important in the analysis and could introduce spurious signals.