F. Couchot

TL;DR: In this article, the authors discuss the Galactic foreground emission between 20 and 100 GHz based on observations by Planck and WMAP, and identify a number of new faint features in the polarized sky, including a dearth of polarized synchrotron emission directly correlated with a narrow, roughly 20deg long filament seen in Hα at high latitude.

TL;DR: In this paper, the authors reported the first measurement of this velocity signature using the aberration and modulation on the CMB temperature anisotropies, finding a component in the known dipole direction.

TL;DR: The Planck Catalogue of Galactic Cold Clumps (PGCC) as mentioned in this paper is an all-sky catalogue of Galactic cold clump candidates detected by Planck, which contains 13,188 sources spread across the whole sky, following the spatial distribution of the main molecular cloud complexes.

TL;DR: In this article, the authors measured the anomalous and aberration and modulation effects on the CMB temperature anisotropies, finding a component in the known dipole direction, (l,b)=(264, 48) [deg], of 384km/s +- 78km/σ +- 115km/ss (syst.).

TL;DR: In this article, the authors make use of the Planck 353 GHz I, Q, and U Stokes maps as dust templates, and cross-correlate them with the WMAP data at 12 frequencies from 23 to 353 GHz, over circular patches with 10 degree radius.