Complementing the ground-based CMB-S4 experiment on large scales with the PIXIE satellite
E Calabrese, D Alonso, J Dunkley - Physical Review D, 2017 - APS
We present forecasts for cosmological parameters from future cosmic microwave
background (CMB) data measured by the stage-4 (S4) generation of ground-based …
background (CMB) data measured by the stage-4 (S4) generation of ground-based …
External priors for the next generation of CMB experiments
Planned cosmic microwave background (CMB) experiments will improve what we know
about neutrino physics, inflation, and dark energy. The low level of noise, together with …
about neutrino physics, inflation, and dark energy. The low level of noise, together with …
Mitigating the optical depth degeneracy using the kinematic Sunyaev-Zel'dovich effect with CMB-S4 data
The epoch of reionization is one of the major phase transitions in the history of the universe,
and is a focus of ongoing and upcoming cosmic microwave background (CMB) experiments …
and is a focus of ongoing and upcoming cosmic microwave background (CMB) experiments …
CMB-S4 technology book
CMB-S4 is a proposed experiment to map the polarization of the Cosmic Microwave
Background (CMB) to nearly the cosmic variance limit for angular scales that are accessible …
Background (CMB) to nearly the cosmic variance limit for angular scales that are accessible …
Optimization study for the experimental configuration of CMB-S4
Abstract The CMB Stage 4 (CMB-S4) experiment is a next-generation, ground-based
experiment that will measure the cosmic microwave background (CMB) polarization to …
experiment that will measure the cosmic microwave background (CMB) polarization to …
A projected estimate of the reionization optical depth using the CLASS experiment's sample variance limited e-mode measurement
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 …
experiment and recover a nearly cosmic variance limited estimate of the reionization optical …
Reconstructing CMB fluctuations and the mean reionization optical depth
PD Meerburg, J Meyers, KM Smith, A Van Engelen - Physical Review D, 2017 - APS
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 …
of primordial fluctuations, and hence in measuring physics that affects the low-redshift …
Towards a cosmological neutrino mass detection
Future cosmological measurements should enable the sum of neutrino masses to be
determined indirectly through their effects on the expansion rate of the Universe and the …
determined indirectly through their effects on the expansion rate of the Universe and the …
Lensing power spectrum of the cosmic microwave background with deep polarization experiments
Precise reconstruction of the cosmic microwave background lensing potential can be
achieved with deep polarization surveys by iteratively removing lensing-induced B modes …
achieved with deep polarization surveys by iteratively removing lensing-induced B modes …
Eliminating the optical depth nuisance from the CMB with 21 cm cosmology
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 …
(CMB) observations, the optical depth τ stands out as a nuisance parameter. While τ …