Monique Arnaud

TL;DR: In this article, the authors present a general methodology to study the dust-Hi correlation over the sky, including simulations to quantify uncertainties, and identify a Galactic contribution to these residuals with variations of the dust emissivity on angular scales smaller than that of their correlation analysis.

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: The Planck Catalogue of Galactic Cold Clumps (PGCC) as discussed by the authors is an all-sky catalogue of Galactic cold clump candidates detected by Planck and contains 13,188 sources spread across the whole sky, i.e., from the Galactic plane to high latitudes, following the spatial distribution of the main molecular cloud complexes.

TL;DR: In this paper, the ISW effect was detected using CMB maps from the 2013 Planck mission data release, and the significance of detection ranges from 2 to 4 sigma, depending on which method is used.

TL;DR: In this article, the scaling relation between Sunyaev-Zeldovich (SZ) signal and stellar mass for almost 260,000 locally brightest galaxies (LBGs) selected from the Sloan Digital Sky Survey (SDSS) was presented.