activity
20182020
most citedHunting for Galaxies and Halos in simulations with VELOCIraptor

100 citations · 163 across the 2 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2020

The BUFFALO HST Survey

Charles L. Steinhardt, Mathilde Jauzac, Ana Acebron +91

The Beyond Ultra-deep Frontier Fields and Legacy Observations (BUFFALO) is a 101 orbit + 101 parallel Cycle 25 Hubble Space Telescope Treasury program taking data from 2018-2020. B…

astro-ph.GA2019

From Stellar Halos to Intracluster Light: the physics of the Intra-Halo Stellar Component in cosmological hydrodynamical simulations

Rodrigo Cañas, Claudia del P. Lagos, Pascal J. Elahi +4

We study the Intra-Halo Stellar Component (IHSC) of Milky Way-mass systems up to galaxy clusters in the Horizon-AGN cosmological hydrodynamical simulation. We identify the IHSC usi…

astro-ph.CO2019100 cited

Hunting for Galaxies and Halos in simulations with VELOCIraptor

Pascal J. Elahi, Rodrigo Cañas, Rhys J. J. Poulton +5

We present VELOCIraptor, a massively parallel galaxy/(sub)halo finder that is also capable of robustly identifying tidally disrupted objects and separate stellar halos from galaxie…

astro-ph.IM2019

Climbing Halo Merger Trees with TreeFrog

Pascal J. Elahi, Rhys J. J. Poulton, Rodrigo J. Tobar +4

We present TreeFrog, a massively parallel halo merger tree builder that is capable comparing different halo catalogues and producing halo merger trees. The code is written in c++11…

astro-ph.GA2018

The Three Hundred project: a large catalogue of theoretically modelled galaxy clusters for cosmological and astrophysical applications

Weiguang Cui, Alexander Knebe, Gustavo Yepes +34

We introduce the THE THREE HUNDRED project, an endeavour to model 324 large galaxy clusters with full-physics hydrodynamical re-simulations. Here we present the data set and study…

astro-ph.GA2018

Introducing a new, robust galaxy finder algorithm for simulations

Rodrigo Cañas, Pascal J. Elahi, Charlotte Welker +4

Identifying galaxies in hydrodynamical simulations is a difficult task, particularly in regions of high density such as galaxy groups and clusters. We present a new scale-free shap…