SUMMARY
PICO will measure polarization anisotropies with high fidelity, specifically focusing on E-mode anisotropies and the low-multipole B modes critical for cosmology. The PICO science paper indicates that full-sky Compton-y maps will be produced, primarily limited to l=1000, yet the satellite's angular resolution allows for kSZ temperature anisotropy measurements at l=3000. Key requirements for accurate B-mode measurements include multiple frequency bands and stringent control of systematic errors, as high multipoles are dominated by noise from lensing residuals.
PREREQUISITES
- Understanding of polarization anisotropies in cosmology
- Familiarity with Compton-y maps and their significance
- Knowledge of E-mode and B-mode polarization signals
- Awareness of systematic errors in astronomical measurements
NEXT STEPS
- Research the methodology for measuring E-mode and B-mode polarization signals
- Explore the impact of lensing on polarization measurements in cosmology
- Study the design and capabilities of satellite instruments for cosmic microwave background observations
- Investigate techniques for controlling systematic errors in astrophysical data analysis
USEFUL FOR
Astronomers, cosmologists, and researchers involved in cosmic microwave background studies, particularly those focusing on polarization measurements and systematic error management.