G. Maggio

TL;DR: In this paper, the authors present a description of the pipeline used to calibrate the Planck Low Frequency Instrument (LFI) timelines into thermodynamic temperatures for the planck 2015 data release, covering four years of uninterrupted operations.

TL;DR: In this paper, the beam normalization and beam window functions for the Planck Low Frequency Instrument (LFI) were characterized and the uncertainties in the beam window function were analyzed.

TL;DR: In this paper, the authors describe the processing of data from the Low Frequency Instrument (LFI) used in production of the Planck Early Release Compact Source Catalogue (ERCSC), in particular, the steps involved in reducing the data from telemetry packets to cleaned, calibrated, time-ordered data (TOD) and frequency maps.

TL;DR: In this article, the Stokes I, Q, and U maps of the Planck satellite were used to study the statistical properties of interstellar dust polarization at high Galactic latitudes around the south pole (b < −60°).

TL;DR: Montier et al. as mentioned in this paper used the Planck-HFI 2015 data release at high frequencies to place new constraints on the properties of the polarized thermal dust emission at high Galactic latitudes.