activity
20202026
most citedLCDM halo substructure properties revealed with high resolution and large volume cosmological simulations

35 citations · 63 across the 6 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2026

Galaxies at z > 10: ΛCDM predicts increased Star Formation Efficiency

Francisco Prada, Peter Behroozi, Tomoaki Ishiyama +4

We show that the rest-frame UV statistics and global properties of galaxies at 7 <= z <= 14 are naturally reproduced within the standard ΛCDM framework when galaxy formation is mod…

astro-ph.CO2025★ 1 cited

A redshift-independent theoretical halo mass function validated with Uchuu simulations

Elena Fernández-García, Juan E. Betancort-Rijo, Francisco Prada +3

We present a new theoretical framework for the halo mass function (HMF) that accurately predicts the abundance of dark matter haloes across an exceptionally wide range in mass and…

astro-ph.GA2022★ 23 cited

The Uchuu-UniverseMachine dataset: Galaxies in and around Clusters

Han Aung, Daisuke Nagai, Anatoly Klypin +7

We present the public data release of the Uchuu-UM galaxy catalogues by applying the UniverseMachine algorithm to assign galaxies to the dark matter halos in the Uchuu -body cos…

astro-ph.CO2022★ 1 cited

The Uchuu-SDSS galaxy lightcones: a clustering, RSD and BAO study

C. A. Dong-Páez, A. Smith, A. O. Szewciw +11

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 particle -body simulation using…

astro-ph.GA2022★ 3 cited

Uchuu-GC galaxies and AGN: Cosmic variance forecasts of high-redshift AGN for JWST, Euclid, and LSST

Taira Oogi, Tomoaki Ishiyama, Francisco Prada +10

Measurements of the luminosity function of active galactic nuclei (AGN) at high redshift () are expected to suffer from field-to-field variance, including cosmic and Po…

astro-ph.CO2021★ 35 cited

LCDM halo substructure properties revealed with high resolution and large volume cosmological simulations

Ángeles Moliné, Miguel A. Sánchez-Conde, Alejandra Aguirre-Santaella +8

We investigate the structural properties, distribution and abundance of LCDM dark matter subhaloes using the Phi-4096 and Uchuu suite of N-body cosmological simulations. Thanks to…