Precise reconstruction of the cosmic microwave background lensing potential can be
achieved with deep polarization surveys by iteratively removing lensing-induced B modes …

Deep surveys of the CMB polarization have more information on the lensing signal than the
quadratic estimators (QE) can capture. We showed in a recent work that a CMB lensing …

The cosmic microwave background (CMB) lensing power spectrum is a powerful probe of
the late-time Universe, encoding valuable information about cosmological parameters such …

We discuss the non-Gaussian contribution to the power spectrum covariance of cosmic
microwave background (CMB) anisotropies resulting through weak gravitational lensing …

Gravitational lensing of the cosmic microwave background (CMB) is a valuable
cosmological signal that correlates to tracers of large-scale structure and acts as a important …

Future low-noise cosmic microwave background (CMB) lensing measurements from eg,
CMB-S4 will be polarization dominated, rather than temperature dominated. In this new …

The power spectrum of cosmic microwave background lensing is a powerful tool for
constraining fundamental physics such as the sum of neutrino masses and the dark energy …

We analyze the possibility of delensing cosmic microwave background (CMB) polarization
maps using foreground weak lensing (WL) information. We build an estimator of the CMB …

Lensing reconstruction maps from the cosmic microwave background (CMB) provide direct
observations of the matter distribution of the universe without the use of a biased tracer …

Gravitational lensing due to the large-scale distribution of matter in the cosmos distorts the
primordial cosmic microwave background (CMB) and thereby induces new, small-scale B …