C A Dong-Páez   A Smith   A O Szewciw   J Ereza   M H Abdullah   C Hernández-Aguayo   S Trusov   F Prada   A Klypin   T Ishiyama   A Berlind   P Zarrouk   J López Cacheiro   J Ruedas   
Monthly Notices of the Royal Astronomical Society Jan 2024 [Refereed]
Abstract
We present the data release of the Uchuu-SDSS galaxies: a set of 32 high-fidelity galaxy lightcones constructed from the large Uchuu 2.1 trillion particles N-body simulation using Planck cosmology. We adopt subhalo abundance matching to...
Monthly Notices of the Royal Astronomical Society Dec 2023 [Refereed]
Abstract
Gravitational N-body simulations calculate numerous interactions between particles. The tree algorithm reduces these calculations by constructing a hierarchical oct-tree structure and approximating gravitational forces on particles. Ove...
Mohamed H Abdullah   Anatoly Klypin   Francisco Prada   Gillian Wilson   Tomoaki Ishiyama   Julia Ereza   
Monthly Notices of the Royal Astronomical Society: Letters 529(1) L54-L59 Dec 2023 [Refereed]
ABSTRACT
We measure the two-point correlation function (CF) of 1357 galaxy clusters with a mass of log10M200 ≥ 13.6 h−1 M⊙ and at a redshift of z ≤ 0.125. This work differs from previous analyses in that it utilizes a spectroscopic cluster catal...
Julia Ereza   Francisco Prada   Anatoly Klypin   Tomoaki Ishiyama   Alex Smith   Carlton M. Baugh   Baojiu Li   César Hernández-Aguayo   José Ruedas   
Nov 2023
Cosmologists aim to uncover the underlying cosmological model governing the
formation and evolution of the Universe. One approach is through studying the
large-scale structure (LSS) traced by galaxy redshift surveys. In this paper,
we explore clus...
Taira Oogi   Tomoaki Ishiyama   Francisco Prada   Manodeep Sinha   Darren Croton   Sofía A Cora   Eric Jullo   Anatoly A Klypin   Masahiro Nagashima   J López Cacheiro   José Ruedas   Masakazu A R Kobayashi   Ryu Makiya   
Monthly Notices of the Royal Astronomical Society 525(3) 3879-3895 Sep 2023 [Refereed]
ABSTRACT
Measurements of the luminosity function of active galactic nuclei (AGN) at high redshift (z ≳ 6) are expected to suffer from field-to-field variance, including cosmic and Poisson variances. Future surveys, such as those from the Euclid ...