D. Santos

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 relationship between the thermal Sunyaev-Zeldovich (SZ) signal and X-ray luminosity is investigated and the measured SZ signal is compared to values predicted from Xray data, underlining the robustness and consistency of the overall view of intra-cluster medium properties.

TL;DR: In this paper, a spectral energy distribution (SED) was created for various Galactocentric radii using velocity information from atomic (neutral hydrogen) and molecular ((12)CO) observations.

TL;DR: Xspect as discussed by the authors is a method to obtain estimates of the angular power spectrum of the cosmic microwave background (CMB) temperature anisotropies including analytical error bars developed for the Archeops experiment.