collaborators

9 papers

astro-ph.CO2026

Sensitivity of Next-Generation CMB Surveys to Neutrinos and Other Light Relics

Cynthia Trendafilova, Srinivasan Raghunathan, Benjamin Wallisch +33

Neutrinos and other light relics leave characteristic imprints in the cosmic microwave background anisotropies, making their observation a sensitive probe of the particle content a…

astro-ph.IM2026

Atmosphere mitigation in CMB observations using multi-frequency time-domain component separation

Julien Tang, Shamik Ghosh, Jacques Delabrouille +4

CMB observations from ground-based observatories are limited in sensitivity by the fluctuating emission from the Earth's atmosphere, mostly due to water vapor inhomogeneities. Even…

astro-ph.CO2026

Unbiased Primordial Gravitational Wave Inference from the CMB with SMICA

Alexander Steier, Shamik Ghosh, Jacques Delabrouille

The detection of primordial gravitational waves in Cosmic Microwave Background B-mode polarization observations requires accurate and robust subtraction of astrophysical contaminat…

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.CO2025

Full-sky Models of Galactic Microwave Emission and Polarization at Sub-arcminute Scales for the Python Sky Model

Experiment Galactic Science Group, Julian Borrill, Susan E. Clark +15

Polarized foreground emission from the Galaxy is one of the biggest challenges facing current and upcoming cosmic microwave background (CMB) polarization experiments. We develop ne…

astro-ph.IM2025

Fast far-sidelobe modeling for centimeter to sub-millimeter astrophysical observations

Oliver Jeong, Jacques Delabrouille, Michel Piat

Next-generation centimeter to sub-millimeter telescopes require exquisite control over instrumental far-sidelobe response to accurately measure faint signals like the Cosmic Microw…