Abstract
We present efficient algorithms for cosmic microwave background (CMB) lensing simulation and power spectrum estimation for flat-sky CMB polarization maps. We build a pure B-mode estimator to remedy E to B leakage due to partial sky coverage. We show that our estimators are unbiased, and consistent with the projected errors. We demonstrate our algorithm using simulated observations of small sky patches with realistic noise and weights for upcoming CMB polarization experiments.
Original language | English (US) |
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Pages (from-to) | 2040-2047 |
Number of pages | 8 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 435 |
Issue number | 3 |
DOIs | |
State | Published - Nov 2013 |
Externally published | Yes |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science
Keywords
- cosmic background radiation