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

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

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

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 ...

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

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

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.

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.

In most cases, the component sepa- ration methods use frequency channel maps as input, with the exception of the temperature analysis performed by Commander,.

Planck 2015 results. X. Diffuse component separation: Foreground maps ; Type. Journal Article ; Keywords. cosmic background radiation, cosmology: observations, ...