activity
20132023
most citedThe BACCO Simulation Project: Exploiting the full power of large-scale structure for cosmology

199 citations · 2.6k across the 48 of their papers we have counts for

collaborators
Showing 2021Show all

6 papers · 1 filter

astro-ph.CO2021★ 37 cited

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.CO2021★ 22 cited

Modelling galaxy clustering in redshift space with a Lagrangian bias formalism and -body simulations

Marcos Pellejero-Ibanez, Jens Stuecker, Raul E. Angulo +3

Improving the theoretical description of galaxy clustering on small scales is an important challenge in cosmology, as it can considerably increase the scientific return of forthcom…

astro-ph.CO2021★ 1 cited

Predicting halo occupation and galaxy assembly bias with machine learning

Xiaoju Xu, Saurabh Kumar, Idit Zehavi +1

Understanding the impact of halo properties beyond halo mass on the clustering of galaxies (namely galaxy assembly bias) remains a challenge for contemporary models of galaxy clust…

astro-ph.CO2021★ 42 cited

Non-universality of the mass function: dependence on the growth rate and power spectrum shape

Lurdes Ondaro-Mallea, Raul E. Angulo, Matteo Zennaro +2

The abundance of dark matter haloes is one of the key probes of the growth of structure and expansion history of the Universe. Theoretical predictions for this quantity usually ass…

astro-ph.CO2021★ 55 cited

The BACCO simulation project: biased tracers in real space

Matteo Zennaro, Raul E. Angulo, Marcos Pellejero-Ibáñez +3

We present an emulator for the two-point clustering of biased tracers in real space. We construct this emulator using neural networks calibrated with more than cosmological m…

astro-ph.GA2021★ 24 cited

SHAM through the lens of a hydrodynamical simulation

Ginevra Favole, Antonio D. Montero-Dorta, M. Celeste Artale +3

We use the IllustrisTNG100 hydrodynamical simulation to study the dependence of the galaxy two-point correlation function on a broad range of secondary subhalo and galactic propert…