CMB B-mode - NEXT

Galactic Foregrounds and Component Separation

28 janv. 2025, 13:30

2h

Seminar Hall (KEK, Tsukuba - Building 3)

Sous-contributions

• Foreground modeling for CMB B-modes observations: Synchrotron emission
• Modelling of the polarized thermal dust signal: review and prospects
• Component separation with no (few) assumptions: ILC methods
• Foreground cleaning - Minimally informed component separation
• Systematic Effect Mitigation in Parametric Component Separation
• Foreground Cleaning - Delta Maps
• Discussion: Current Priorities on Foreground Cleaning and Modeling