78 citations · 78 across the 1 of their papers we have counts for
7 papers
The better half -- Asymmetric star-formation due to ram pressure in the EAGLE simulations
P. Troncoso-Iribarren, N. Padilla, C. Santander +4
We use the EAGLE simulations to study the effects of the intra-cluster medium (ICM) on the spatially resolved star-formation activity in galaxies. We study three cases of galaxy as…
Do model emission line galaxies live in filaments at z~1?
V. Gonzalez-Perez, W. Cui, S. Contreras +7
Current and future cosmological surveys are targeting star-forming galaxies at with nebular emission lines. We use a state-of-the-art semi-analytical model of galaxy form…
Modelling the large scale structure of the Universe as a function of cosmology and baryonic physics
Giovanni Aricò, Raul E. Angulo, Carlos Hernández-Monteagudo +4
We present and test a framework that models the three-dimensional distribution of mass in the Universe as a function of cosmological and astrophysical parameters. Our approach comb…
On the prospect of using the maximum circular velocity of halos to encapsulate assembly bias in the galaxy-halo connection
Idit Zehavi, Stephen E. Kerby, Sergio Contreras +3
We investigate a conceptual modification of the halo occupation distribution approach, using the halos' present-day maximal circular velocity, $\vmax$, as an alternative to halo ma…
Extensions to the halo occupation distribution model for more accurate clustering predictions
Esteban Jiménez, Sergio Contreras, Nelson Padilla +3
We test different implementations of the halo occupation distribution (HOD) model to reconstruct the spatial distribution of galaxies as predicted by a publicly available semi-anal…
How to add massive neutrinos to your CDM simulation -- extending cosmology rescaling algorithms
Matteo Zennaro, Raúl E. Angulo, Giovanni Aricò +2
Providing accurate predictions for the spatial distribution of matter and luminous tracers in the presence of massive neutrinos is an important task, given the imminent arrival of…