Jun 22, 2015 · We discuss the Galactic foreground emission between 20 and 100GHz based on observations by Planck/WMAP.

We discuss the Galactic foreground emission between 20 and 100 GHz based on observations by Planck and WMAP. The total intensity in this part of the spectrum is ...

Abstract. We discuss the Galactic foreground emission between 20 and 100 GHz based on observations by Planck and WMAP. The total intensity in this part of ...

Planck 2015 results. XXV. Diffuse low-frequency Galactic foregrounds ... Galactic plane. Comparison of the high-latitude Hα emission with our free-free map ...

Planck 2015 results. Special feature. Planck 2015 results. XXV. Diffuse low-frequency Galactic foregrounds. Planck Collaboration: P. A. R. Ade95, N. Aghanim64 ...

(abridged) We discuss the Galactic foreground emission between 20 and 100GHz based on observations by Planck/WMAP. The Commander component-separation tool ...

Planck 2015 results. XXV. Diffuse low-frequency Galactic foregrounds. Author. Planck Collaboration, P. A. R. Ade, N. Aghanim, M. I. R. Alves, M. Arnaud, M ...

In this paper, we discuss the Galactic foreground emission between 20 and 100 GHz based on observations by Planck and WMAP. The total intensity in this part ...

We discuss the Galactic foreground emission between 20 and 100 GHz based on observations by Planck and WMAP.

We discuss the Galactic foreground emission between 20 and 100 GHz based on observations by Planck and WMAP. The total intensity in this part of the spectrum is ...