collaborators

5 papers

astro-ph.CO2025

An iterative CMB lensing estimator minimizing instrumental noise bias

Louis Legrand, Blake Sherwin, Anthony Challinor +2

Noise maps from CMB experiments are generally statistically anisotropic, due to scanning strategies, atmospheric conditions, or instrumental effects. Any mis-modeling of this compl…

astro-ph.CO2025

Characterizing CMB noise anisotropies from CMB delensing

Louis Legrand, Julien Carron

Un-doing the effect of gravitational lensing on the Cosmic Microwave Background (`de-lensing') is essential in shaping constraints on weak signals limited by lensing effects on the…

astro-ph.CO2025

On likelihood-based analysis of the gravitationally (de)lensed CMB

Julien Carron

By reducing variance induced by gravitational lensing, likelihood-based de-lensing techniques have true potential to extract significantly more information from deep and high-resol…

astro-ph.CO2025

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves

Federico Bianchini, Dominic Beck, W. L. Kimmy Wu +6

We compare multiple foreground-cleaning pipelines for estimating the tensor-to-scalar ratio, , using simulated maps of the planned CMB-S4 experiment within the context of the So…

astro-ph.CO2025

Detecting rotation from lensing in the CMB

Julien Carron, Enea di Dio, Ruth Durrer

An excellent estimate of the lensing signal is expected from the availability of deep and high-resolution polarization data in the near future. This is most important to allow for…