most citedJWST imaging of the Pleiades: anisotropy of turbulence in the cold neutral medium

1 citations · 1 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2026

Status of the COSmological Microwave Observations CALibrator

L. Mousset, J. Aumont, S. Berta +33

As the sensitivity of CMB telescopes increases, the need for precise calibration becomes critical. Started in 2022, the COSMOCal project aims to place an artificial polarized sourc…

astro-ph.GA20261 cited

JWST imaging of the Pleiades: anisotropy of turbulence in the cold neutral medium

G. Vigoureux, N. Flagey, F. Boulanger +14

Interstellar medium studies rely on magnetohydrodynamic (MHD) turbulence as a framework for interpretation. In this context, the statistical characterization of interstellar observ…

astro-ph.GA2023

All We Are Is Dust In The WIM: Constraints on Dust Properties in the Milky Way's Warm Ionized Medium

J. L. West, B. M. Gaensler, M. -A. Miville-Deschênes +5

We present a comparison of the presence and properties of dust in two distinct phases of the Milky Way's interstellar medium: the warm neutral medium (WNM) and the warm ionized med…

astro-ph.IM2023

Polarization angle accuracy for future CMB experiments. The COSMOCal project and its prototype in the 1mm band

A. Ritacco, L. Bizzarri, F. Boulanger +24

The Cosmic Microwave Background (CMB) radiation offers a unique window into the early Universe, facilitating precise examinations of fundamental cosmological theories. However, the…

astro-ph.CO2023

Wavelet Based Statistics for Enhanced 21cm EoR Parameter Constraints

Ian Hothi, Erwan Allys, Benoit Semelin +1

We propose a new approach to improve the precision of astrophysical parameter constraints for the 21cm signal from the epoch of reionisation (EoR). Our method introduces new sets o…

astro-ph.GA2023

Bayesian inference methodology to characterize the dust emissivity at far-infrared and submillimeter frequencies

Debabrata Adak, Shabbir Shaikh, Srijita Sinha +5

We present a Bayesian inference method to characterise the dust emission properties using the well-known dust-HI correlation in the diffuse interstellar medium at Planck frequencie…