Feb 5, 2015 · In this paper we consider the problem of diffuse astrophysical component separation, and process these maps within a Bayesian framework to ...

In this paper we consider the problem of diffuse astrophysical component separation, and process these maps within a Bayesian framework to derive an internally ...

Diffuse component separation: Foreground maps. Planck has mapped the microwave sky in temperature over nine frequency bands between 30 and 857 GHz and in ...

Planck has mapped the microwave sky in nine frequency bands between 30 and 857 GHz in temperature and seven bands between 30 and 353 GHz in polarization.

Abstract. Planck has mapped the microwave sky in temperature over nine frequency bands between 30 and 857 GHz and in polarization over seven frequency bands ...

Authors Planck Collaboration • Adam, R. Ade, P. A. R. · Abstract Planck has mapped the microwave sky in temperature over nine frequency bands between 30 and ...

Mar 8, 2017 · In this paper we consider the problem of diffuse astrophysical component separation, and process these maps within a Bayesian framework to ...

Feb 20, 2015 · Abstract:We present foreground-reduced CMB maps derived from the full Planck data set in both temperature and polarization.

Planck 2015 results X. Diffuse component separation: Foreground maps ; Authors. Nabila Aghanim · Monique Arnaud · Jonathan Aumont · Bruce Partridge, Haverford ...

In this paper we consider the problem of diffuse astrophysical component separation, and process these maps within a Bayesian framework to derive a consistent ...