We analyze simulated maps of the Cosmology Large Angular Scale Surveyor (CLASS)
experiment and recover a nearly cosmic variance limited estimate of the reionization optical …

The Thomson optical depth from reionization is a limiting factor in measuring the amplitude
of primordial fluctuations, and hence in measuring physics that affects the low-redshift …

We investigate the impact of instrumental systematic errors on the potential of cosmic
microwave background polarization experiments targeting primordial B-modes. To do so, we …

We present forecasts for cosmological parameters from future cosmic microwave
background (CMB) data measured by the stage-4 (S4) generation of ground-based …

We study the possibility of measuring the optical depth at reionization τ without relying on
large-scale cosmic microwave background (CMB) polarization. Our analysis is driven by the …

We consider the effectiveness of foreground cleaning in the recovery of Cosmic Microwave
Background (CMB) polarization sourced by gravitational waves for tensor-to-scalar ratios in …

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

Amongst standard model parameters that are constrained by cosmic microwave background
(CMB) observations, the optical depth τ stands out as a nuisance parameter. While τ …

We explore the fundamental limits to which reionization histories can be constrained using
only large-scale cosmic microwave background (CMB) anisotropy measurements. The …

Cosmic microwave background (CMB) polarization observations will require superb control
of systematic errors in order to achieve their full scientific potential, particularly in the case of …