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From the 1 of 7 linked papers with an AI index.

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7 papers

astro-ph.IM2026

Proof of concept of the COSMOCal project at the IRAM 30m telescope

S. Savorgnano, L. Bizzarri, A. Ritacco +25

This work reports on a test campaign conducted at the IRAM 30m telescope to validate the COSMOCal instrument, a novel concept for absolute calibration of polarization angle, beam p…

astro-ph.IM2026

Status and future development of the COSMOCal Project for absolute CMB polarization calibration

Silvia Micheli, Alessia Ritacco, Alessandro Carones +36

The paper outlines the COSMOCal project, which will place an artificial polarized microwave source on a geostationary satellite to provide stable absolute calibration for CMB polar…

astro-ph.GA2026

Untangling dust emission and cosmic infrared background anisotropies with the scattering transform statistics

Srijita Sinha, Tuhin Ghosh, Erwan Allys +2

The template-fit approach is often used to separate Galactic dust emission from cosmic infrared background (CIB) anisotropies in low column density regions, under the a…

astro-ph.GA2026

The multiphase interstellar medium as a common origin for magnetic misalignment and TB parity violation

Andrea Bracco, Ari J. Cukierman, Raphael Skalidis +1

We present an original data analysis and a physical model that provide new insights into the origin of, and relationship between, two observables of the dusty, polarized Galaxy at…

astro-ph.CO2026

Separation of polarized dust emission in Planck observations with Scattering Transforms

Alexandros Tsouros, Elisa Russier, Erwan Allys +3

Polarized dust emission is a major astrophysical foreground contaminant of the cosmic microwave background polarization (CMB), which must be accurately measured to look for the fai…

astro-ph.GA2025

Variance of dust temperature and spectral index in Planck polarization data using spin-moment expansion

Vincent Guillet, Léo Vacher, Jonathan Aumont +4

Thermal dust is the major polarized foreground hindering the detection of primordial cosmic microwave background (CMB) B-modes. Its signal exhibits complex behavior in frequency sp…