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 ...

We discuss in detail the large-scale features in the low frequency polarized sky including the well-known loops and spurs. Other results will be published in ...

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 ...

The scientific results that we present today are a product of the Planck Collaboration, including individuals from more than 100 scientific institutes in Europe ...

Planck Collaboration (2016). Planck 2015 results XXV. Diffuse low-frequency Galactic foregrounds. Astronomy &. Astrophysics, 594. https://doi.org/10.1051 ...

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 the ...

Planck 2015 results. XXV. Diffuse low-frequency Galactic foregrounds. A&A (in publication), arXiv: 1506.06660. Corresponding authors: Clive Dickinson, Paddy ...

The region in light blue shows where the AME at 22.8\GHz is brighter than 1\,mK; this is also masked when determining the best-fitting emissivity.

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 ...