Simultaneous inference of isotropic and anisotropic polarization rotation angles for next-generation cosmic microwave background experiments
Yue Zhang, Chang Feng, Sen Li, Filipe B. Abdalla
astro-ph.CO
Submitted: 2026-07-20
Comments: 18 pages, 9 figures
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Quintessence and the Rest of the World
- Self-Calibration of BICEP1 Three-Year Data and Constraints on Astrophysical Polarization Rotation
- Probing CPT Violation with CMB Polarization Measurements
- POLARBEAR Constraints on Cosmic Birefringence and Primordial Magnetic Fields
- BICEP / Keck XVII: Line of Sight Distortion Analysis: Estimates of Gravitational Lensing, Anisotropic Cosmic Birefringence, Patchy Reionization, and Systematic Errors
- The Atacama Cosmology Telescope: Constraints on Cosmic Birefringence
- Planck intermediate results. L. Evidence for spatial variation of the polarized thermal dust spectral energy distribution and implications for CMB $B$-mode analysis
- Is cosmic birefringence due to dark energy or dark matter? A tomographic approach
- Faraday Rotation of Microwave Background Polarization by a Primordial Magnetic Field
- Axion Dark Matter Detection with CMB Polarization
- Self-Calibration of CMB Polarization Experiments
- New Extraction of the Cosmic Birefringence from the Planck 2018 Polarization Data
- Cosmic Birefringence from Planck Data Release 4
- Improved Constraints on Cosmic Birefringence from the WMAP and Planck Cosmic Microwave Background Polarization Data
- Cosmic Birefringence from the Atacama Cosmology Telescope Data Release 6
- The Simons Observatory: Science Goals and Forecasts for the Enhanced Large Aperture Telescope
- Characterization of the Polarization Beam Response of SPT-3G Using Point Sources
- Peeling off foregrounds with the constrained moment ILC method to unveil primordial CMB $B$-modes
- Optimization of foreground moment deprojection for semi-blind CMB polarization reconstruction
- Inference of $B$-mode polarization in the presence of non-Gaussian foregrounds
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