J. Knoche

TL;DR: The Planck Catalogue of Compact Sources (PCCS) as mentioned in this paper is the catalogue of sources detected in the first 15 months of Planck operations, the "nominal" mission, which consists of nine single-frequency catalogues of compact sources, both Galactic and extragalactic, detected over the entire sky.

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

TL;DR: The Planck Catalogue of Compact Sources (PCCS) as mentioned in this paper is the catalogue of sources detected in the first 15 months of Planck operations, the "nominal" mission, which consists of nine single-frequency catalogues of compact sources, both Galactic and extragalactic, detected over the entire sky.

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.