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arxiv 1301.4145 v1 pith:YDDLIMDL submitted 2013-01-17 astro-ph.CO

Full-sky CMB lensing reconstruction in presence of sky-cuts

Aur\'elien Benoit-L\'evy , Typhaine D\'echelette , Karim Benabed , Jean-Fran\c{c}ois Cardoso , Duncan Hanson , Simon Prunet This is my paper
classification astro-ph.CO
keywords lensingreconstructiongalacticpointpotentialpowerpresencesky-cuts
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We consider the reconstruction of the CMB lensing potential and its power spectrum of the full sphere in presence of sky-cuts due to point sources and Galactic contaminations. Those two effects are treated separately. Small regions contaminated by point sources are filled in using Gaussian constrained realizations. The Galactic plane is simply masked using an apodized mask before lensing reconstruction. This algorithm recovers the power spectrum of the lensing potential with no significant bias.

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  1. CMB Lensing Reconstruction Using Two Years of Temperature Data from the SPT-3G Summer Survey

    astro-ph.CO 2026-07 conditional novelty 5.0

    First CMB lensing reconstruction from two years of SPT-3G Summer temperature data yields A_comb = 1.015 ± 0.053 over 50 < L < 2000, consistent with Planck 2018 ΛCDM.