We present cosmological results from the measurement of baryon acoustic oscillations
(BAO) in galaxy, quasar and Lyman-α forest tracers from the first year of observations from …

We present new measurements of cosmic microwave background (CMB) lensing over 9400
deg 2 of the sky. These lensing measurements are derived from the Atacama Cosmology …

The recent result of the Dark Energy Spectroscopic Instrument (DESI) in combination with
other cosmological data shows evidence of the evolving dark energy parametrized by the w …

We present an updated analysis of eleven cosmological models that may help reduce the
Hubble tension, which now reaches the 6σ level when considering the latest SH0ES …

Scalar field ϕ CDM models provide an alternative to the standard Λ CDM paradigm, while
being physically better motivated. Dynamical scalar field ϕ CDM models are divided into two …

The evolution of the cluster mass function traces the growth of linear density perturbations,
providing valuable insights into the growth of structures, the nature of dark matter, and the …

Weak galaxy lensing surveys have consistently reported low values of the S 8 parameter
compared to the Planck lambda cold dark matter (ΛCDM) cosmology. Amon & Efstathiou …

Abstract Recent Baryon Acoustic Oscillation (BAO) measurements released by DESI, when
combined with Cosmic Microwave Background (CMB) data from Planck and two different …

Baryon acoustic oscillation data from the first year of the Dark Energy Spectroscopic
Instrument (DESI) provide near percent-level precision of cosmic distances in seven bins …

A bstract The baryon acoustic oscillation (BAO) analysis from the first year of data from the
Dark Energy Spectroscopic Instrument (DESI), when combined with data from the cosmic …