We review the field of collisionless numerical simulations for the large-scale structure of the
Universe. We start by providing the main set of equations solved by these simulations and …

We present a method to flexibly and self-consistently determine individual galaxies' star
formation rates (SFRs) from their host haloes' potential well depths, assembly histories, and …

Abstract The Astropy Project supports and fosters the development of open-source and
openly developed Python packages that provide commonly needed functionality to the …

This paper introduces C olossus, a public, open-source python package for calculations
related to cosmology, the large-scale structure (LSS) of matter in the universe, and the …

The two-point correlation function (2PCF) is the most widely used tool for quantifying the
spatial distribution of galaxies. Since the distribution of galaxies is determined by galaxy …

We present nbodykit, an open-source, massively parallel Python toolkit for analyzing large-
scale structure (LSS) data. Using Python bindings of the Message Passing Interface, we …

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

We introduce a novel approach to boost the efficiency of the importance nested sampling
(INS) technique for Bayesian posterior and evidence estimation using deep learning. Unlike …

We present measurements of the redshift-dependent clustering of a DESI-like luminous red
galaxy (LRG) sample selected from the Legacy Survey imaging data set, and use the halo …

Extremely red quasars, with bolometric luminosities exceeding 10 47 erg s− 1, are a
fascinating high-redshift population that is absent in the local universe. They are the best …