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 the Galactic foreground emission between 20 and 100 GHz based on observations by Planck and WMAP.
Second, low-frequency foregrounds have complicated spectra: at a minimum, we must solve for the amplitudes of free-free emission, synchrotron emission, and AME, ...
Planck 2015 results. XXV. Diffuse low-frequency Galactic foregrounds. A&A (submitted), arXiv: 1506.06660. Mike Peel. Jodrell Bank Centre for Astrophysics ...
Planck 2015 results. XXV. Diffuse low-frequency Galactic foregrounds ... Planck and WMAP. The total intensity in this part of the spectrum is dominated by ...
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 ...
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 ...
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 ...
Jun 26, 2015 · (abridged) We discuss the Galactic foreground emission between 20 and 100GHz based on observations by Planck/WMAP.