We present cosmological constraints from a simulation-based inference (SBI) analysis of
galaxy clustering from the SimBIG forward modeling framework. SimBIG leverages the …

We introduce the AbacusHOD model and present two applications of AbacusHOD and the
AbacusSummit simulations to observations. AbacusHOD is a Halo Occupation Distribution …

The high-redshift galaxy UV luminosity function (UVLF) has become essential for
understanding the formation and evolution of the first galaxies. Yet, UVLFs only measure …

Approximate methods to populate dark-matter haloes with galaxies are of great utility to
galaxy surveys. However, the limitations of simple halo occupation models (HODs) preclude …

To extract information from the clustering of galaxies on non-linear scales, we need to model
the connection between galaxies and haloes accurately and in a flexible manner. Standard …

Recent analyses show that ΛCDM-based models optimized to reproduce the clustering of
massive galaxies overestimate their gravitational lensing by about 30 per cent, the so-called …

We introduce a novel technique for constraining cosmological parameters and galaxy
assembly bias using non-linear redshift-space clustering of galaxies. We scale cosmological …

Efficiently mapping baryonic properties onto dark matter is a major challenge in
astrophysics. Although semianalytic models (SAMs) and hydrodynamical simulations have …

The spatial distribution of galaxies and their gravitational lensing signal offer complementary
tests of galaxy formation physics and cosmology. However, their synergy can only be fully …

We present the first simulation-based inference (SBI) of cosmological parameters from field-
level analysis of galaxy clustering. Standard galaxy clustering analyses rely on analyzing …