S. Galeotta

TL;DR: In this paper, the authors presented new estimates of the brightness temperatures of Jupiter, Saturn, Uranus, and Neptune based on the measurements carried in 2009-2013 by Planck /LFI at 30, 44, and 70 GHz and released to the public in 2018.

TL;DR: The Planck satellite is the third generation of space missions devoted to cosmic microwave background (CMB) measurements as discussed by the authors, which will perform two sky surveys and measure the CMB anisotropies and polarization between 30 and 850 GHz.

TL;DR: In this paper, the Planck Low Frequency Instrument (LFI) was measured during the ground cryogenic test campaign and a set of measured calibration parameters were updated during flight operations through the end of the mission.

TL;DR: The conceptual advantages of the Gibbs sampling approach lies in statistically well-defined error propagation and systematic error correction, and this methodology forms the conceptual basis for the map-making algorithm employed in the BeyondPlanck framework, which implements the first end-to-end Bayesian analysis pipeline for CMB observations.

TL;DR: In this article, the application of high-pass Fourier filters to remove periodic systematic fluctuations from full-sky survey CMB datasets has been investigated and compared with the use of destriping codes to remove the effect of residual 1/f noise from timelines.