The existence of a cosmic neutrino background has been inferred indirectly from
cosmological surveys through its effect on the linear-theory evolution of primordial density …

The effects of gravitational lensing of the cosmic microwave background (CMB) have been
measured at high significance with existing data and will be measured even more precisely …

In recent years, weak lensing of the cosmic microwave background (CMB) has emerged as
a powerful tool to probe fundamental physics, such as neutrino masses, primordial non …

The search for primordial gravitational waves in the cosmic microwave background (CMB)
will soon be limited by our ability to remove the lensing contamination to B-mode …

Upcoming measurements of the small-scale primary cosmic microwave background (CMB)
temperature and polarization power spectra (TT/TE/EE) are anticipated to yield …

We constrain the redshift dependence of gas pressure bias⟨ by P e⟩(bias-weighted
average electron pressure), which characterises the thermodynamics of intergalactic gas …

Clusters of galaxies, being the largest collapsed structures in the universe, offer valuable
insights into the nature of cosmic evolution. Precise calibration of the mass of clusters can be …

The kinetic Sunyaev-Zeldovich (kSZ) effect will be an important source of cosmological and
astrophysical information in upcoming surveys of the cosmic microwave background (CMB) …

Measurements of gravitational lensing of the cosmic microwave background (CMB) hold the
promise of yielding unique insights into cosmology at high redshift. Uncertainties due to …

Spatial variations in the cosmic electron density after reionization generate cosmic
microwave background anisotropies via Thomson scattering, a process known as …