We present a new-generation tool to model and interpret spectral energy distributions
(SEDs) of galaxies, which incorporates in a consistent way the production of radiation and its …

Precision cosmology has recently triggered new attention on the topic of approximate
methods for the clustering of matter on large scales, whose foundations date back to the …

Accurate analyses of present and next-generation cosmological galaxy surveys require new
ways to handle effects of non-linear gravitational structure formation processes in data. To …

We present GLADE+, an extended version of the GLADE galaxy catalogue introduced in our
previous paper for multimessenger searches with advanced gravitational-wave detectors …

The non-linear dynamics of scalar fields coupled to matter and gravity can lead to
remarkable density-dependent screening effects. In this short review, we present the main …

Gravitational wave (GW) sources are an excellent probe of the luminosity distance and offer
a novel measure of the Hubble constant, H 0. This estimation of H 0 from standard sirens …

Abstract The Milky Way is surrounded by 11 'classical'satellite galaxies in a remarkable
configuration: a thin plane that is possibly rotationally supported. Such a structure is thought …

Detecting and measuring a non-Gaussian signature of primordial origin in the density field is
a major science goal of next-generation galaxy surveys. The signal will permit us to …

Faint star-forming galaxies at z∼ 2–3 can be used as alternative background sources to
probe the Lyα forest in addition to quasars, yielding high sightline densities that enable 3D …

We present a comparison of simulation-based inference to full, field-based analytical
inference in cosmological data analysis. To do so, we explore parameter inference for two …