Simon Prunet

TL;DR: In this paper, the authors show that anomalous dust emission is present in the atomic, molecular and dark gas phases throughout the Galactocentricity of the Galactic disk, and the derived dust propeties associated with the dark gas phase are derived but do not allow us to reveal the nature of this phase.

TL;DR: In this article, the integrated Sachs-Wolfe (ISW) effect from the Planck 2015 temperature and polarization data release is investigated from different perspectives, and the authors show that the ISW effect is detected only at ≈3σ, which is similar to the detection level achieved by combining the cross-correlation signal coming from all the galaxy catalogues mentioned above.

TL;DR: Generated at a cost of some 25 million CPU-hours spread across multiple high-performance-computing (HPC) platforms, FFP8 is used to validate and verify analysis algorithms and their implementations, and to remove biases from and quantify uncertainties in the results of analyses of the real data.

TL;DR: In this paper, the angular power spectrum was extracted from cosmic microwave background temperature maps by first estimating the correlation function and then finding the error bars and cross-correlations by using a Monte Carlo approach.

TL;DR: In this paper, the authors investigated the source of the millimetre excess in the spectral energy distribution of the Large Magellanic Cloud (LMC) and Small Magellan Cloud (SMC) using the Planck data.