activity
20162025
most citedThe clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Observational systematics and baryon acoustic oscillations in the correlation function

276 citations · 298 across the 3 of their papers we have counts for

collaborators

21 papers

astro-ph.CO2025

Web-Halo Model (WHM): Accurate non-linear matter power spectrum predictions without free parameters

Samuel Brieden, Florian Beutler, Marcos Pellejero-Ibañez

We present a parameter-free variant of the halo model that significantly improves the precision of matter clustering predictions, particularly in the challenging 1-halo to 2-halo t…

astro-ph.CO2021

Covariance matrices for variance-suppressed simulations

Tony Zhang, Chia-Hsun Chuang, Risa H. Wechsler +9

Cosmological -body simulations provide numerical predictions of the structure of the Universe against which to compare data from ongoing and future surveys, but the growing volu…

astro-ph.CO2021

Priors on Lagrangian bias parameters from galaxy formation modelling

Matteo Zennaro, Raul E. Angulo, Sergio Contreras +2

We study the relations among the parameters of the hybrid Lagrangian bias expansion model, fitting biased auto and cross power spectra up to $k_{\rm max} = 0.7 \, h \, \mathrm{Mpc}…

astro-ph.CO2020

The BACCO Simulation Project: A baryonification emulator with Neural Networks

Giovanni Aricò, Raul E. Angulo, Sergio Contreras +3

We present a neural-network emulator for baryonic effects in the non-linear matter power spectrum. We calibrate this emulator using more than 50,000 measurements in a 15-dimensiona…

astro-ph.CO2020

The BACCO Simulation Project: Exploiting the full power of large-scale structure for cosmology

Raul E. Angulo, Matteo Zennaro, Sergio Contreras +3

We present the BACCO project, a simulation framework specially designed to provide highly-accurate predictions for the distribution of mass, galaxies, and gas as a function of cosm…

astro-ph.CO2020

Cosmological parameter estimation via iterative emulation of likelihoods

Marcos Pellejero-Ibañez, Raul E. Angulo, Giovanni Aricó +3

The interpretation of cosmological observables requires the use of increasingly sophisticated theoretical models. Since these models are becoming computationally very expensive and…