Optimal anisotropic CMB filtering plus a second-stage filter on the reconstructed lensing convergence map reduces lensing power spectrum variance by factor 2-5 relative to isotropic filtering, with up to 30% additional improvement on large scales.
This corresponds to using the filter ( bCfidb⊤ +N )−1 WX , where W is diagonal in pixel space and N is taken to be isotropic
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.CO 1years
2019 1verdicts
ACCEPT 1representative citing papers
citing papers explorer
-
Optimal filtering for CMB lensing reconstruction
Optimal anisotropic CMB filtering plus a second-stage filter on the reconstructed lensing convergence map reduces lensing power spectrum variance by factor 2-5 relative to isotropic filtering, with up to 30% additional improvement on large scales.