activity
20242026
collaborators

9 papers

astro-ph.IM2026

Robust CMB polarisation mapmaking with a rotating half-wave plate

Wuhyun Sohn, Simon Biquard, Josquin Errard +1

We present a novel mapmaking method for obtaining unbiased estimates of CMB polarisation, tailored to modern CMB experiments with a rotating half-wave plate. These experiments are…

astro-ph.CO2026

A GPU-Accelerated JAX Framework for Robust Parametric Component Separation and Clustering Optimization for CMB Polarization Satellites

Wassim Kabalan, Arianna Rizzieri, Wuhyun Sohn +6

We present a novel, JAX-powered implementation of a parametric component-separation method for CMB polarization data, explicitly designed to handle spatially varying foreground Spe…

astro-ph.IM2026

Furax: A Modular JAX Framework for Linear Operators in Astrophysical and Cosmological Data Analysis

Pierre Chanial, Simon Biquard, Wassim Kabalan +10

The Framework for Unified and Robust data Analysis with JAX (Furax) is an open-source Python framework for modeling data acquisition systems and solving inverse problems in astroph…

astro-ph.CO2026

Half-wave-plate non idealities propagated to component separated CMB -modes

Ema Tsang-King-Sang, Josquin Errard, Simon Biquard +4

We assess the impact of non-ideal, continuously rotating half-wave plates (HWPs) on cosmic microwave background (CMB) polarization measurements targeting large angular scale signal…

astro-ph.CO2025

Searching for Cosmological Collider in the Planck CMB Data II: collider templates and Modal analysis

Petar Suman, Dong-Gang Wang, Wuhyun Sohn +2

Signatures of massive particles during inflation are highly informative targets for cosmological experiments. With recent progress on both theoretical and observational frontiers,…

astro-ph.CO2025

How Significant are Cosmological Collider Signals in the Planck Data?

Petar Suman, Dong-Gang Wang, Wuhyun Sohn +2

The search for primordial non-Gaussianities (PNG) is theoretically well motivated but remains observationally challenging. Tight constraints with low significance for the standard…