Abstract The Laser Interferometer Space Antenna (LISA) has two scientific objectives of
cosmological focus: to probe the expansion rate of the universe, and to understand …

Long range scalar fields with a coupling to matter appear to violate known bounds on
gravitation in the solar system and the laboratory. This is evaded thanks to screening …

Euclid is a mission of the European Space Agency that is designed to constrain the
properties of dark energy and gravity via weak gravitational lensing and galaxy clustering. It …

A key component of the Dark Energy Spectroscopic Instrument (DESI) survey validation (SV)
is a detailed visual inspection (VI) of the optical spectroscopic data to quantify key survey …

An observational program focused on the high redshift (2< z< 6) Universe has the
opportunity to dramatically improve over upcoming LSS and CMB surveys on measurements …

Cosmological inference with large galaxy surveys requires theoretical models that combine
precise predictions for large-scale structure with robust and flexible galaxy formation …

We analyse the BOSS DR12 multipoles of the galaxy power spectrum jointly with
measurements of the BAO scale for three different models of dark energy. We use recent …

To fully take advantage of the data provided by large-scale structure surveys, we need to
quantify the potential impact of baryonic effects, such as feedback from active galactic nuclei …

Euclid will be the first space mission to survey most of the extragalactic sky in the 0.95–2.02
µm range, to a 5 σ point-source median depth of 24.4 AB mag. This unique photometric …

We use analytic covariance matrices to carry out a full-shape analysis of the galaxy power
spectrum multipoles from the Baryon Oscillation Spectroscopic Survey (BOSS). We obtain …