activity
20142022
most citedA Joint Analysis of BICEP2/Keck Array and Planck Data

985 citations · 2k across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.IM2022

Status of QUBIC, the Q&U Bolometer for Cosmology

L. Mousset, P. Ade, A. Almela +108

The Q&U Bolometric Interferometer for Cosmology (QUBIC) is a novel kind of polarimeter optimized for the measurement of the B-mode polarization of the Cosmic Microwave Back-ground…

astro-ph.CO2022★ 24 cited

Frequency dependence of the thermal dust ratio and correlation: insights from the spin-moment expansion

Léo Vacher, Jonathan Aumont, François Boulanger +4

The change of physical conditions across the turbulent and magnetized interstellar medium (ISM) induces a 3D spatial variation of the properties of Galactic polarized emission. The…

astro-ph.CO2021

Moment expansion of polarized dust SED: a new path towards capturing the CMB -modes with

L. Vacher, J. Aumont, L. Montier +3

Characterizing the polarized dust emission from our Galaxy will be decisive for the quest for the Cosmic Microwave Background (CMB) primordial -modes. The incomplete modelling o…

astro-ph.CO2016★ 65 cited

Planck intermediate results. L. Evidence for spatial variation of the polarized thermal dust spectral energy distribution and implications for CMB -mode analysis

Planck Collaboration, N. Aghanim, M. Ashdown +156

The characterization of the Galactic foregrounds has been shown to be the main obstacle in the challenging quest to detect primordial B-modes in the polarized microwave sky. We mak…

astro-ph.CO2015★ 985 cited

A Joint Analysis of BICEP2/Keck Array and Planck Data

BICEP2/Keck, Planck Collaborations, : +276

We report the results of a joint analysis of data from BICEP2/Keck Array and Planck. BICEP2 and Keck Array have observed the same approximately 400 deg patch of sky centered on…

astro-ph.GA2014★ 422 cited

Planck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dust

Planck Collaboration, P. A. R. Ade, N. Aghanim +199

This paper presents the large-scale polarized sky as seen by Planck HFI at 353 GHz, which is the most sensitive Planck channel for dust polarization. We construct and analyse large…