activity
20012021
most citedSubhaloes gone Notts: Spin across subhaloes and finders

41 citations · 72 across the 2 of their papers we have counts for

collaborators

10 papers

astro-ph.CO2021

On the weak lensing masses of a new sample of galaxy groups

Elizabeth J. Gonzalez, Facundo Rodriguez, Manuel Merchán +6

Galaxy group masses are important to relate these systems with the dark matter halo hosts. However, deriving accurate mass estimates is particularly challenging for low-mass galaxy…

astro-ph.GA202031 cited

Deviations from tidal torque theory: evolution of the halo spin-filament alignment

Pablo López, Marius Cautun, Dante Paz +2

The alignment between halo spins and the cosmic web is still poorly understood despite being a widely studied topic. Here, we study this alignment within the context of tidal torqu…

astro-ph.GA2020

The galaxy size - halo mass scaling relations and clustering properties of central and satellite galaxies

Facundo Rodriguez, Antonio D. Montero-Dorta, Raul E. Angulo +2

In this work, we combine size and stellar mass measurements from the Sloan Digital Sky Server (SDSS) with the group finder algorithm of Rodriguez \& Merchán in order to determine t…

astro-ph.CO2020

Combining FOF and halo-based algorithms for the identification of galaxy groups

Facundo Rodriguez, Manuel Merchán

Galaxy groups provide the means for a great diversity of studies that contribute to a better understanding of the structure of the universe on a large scale and allow the propertie…

astro-ph.IM2019

GriSPy: A Python package for Fixed-Radius Nearest Neighbors Search

Martin Chalela, Emanuel Sillero, Luis Pereyra +4

We present a new regular grid search algorithm for quick fixed-radius nearest-neighbor lookup developed in Python. This module indexes a set of k-dimensional points in a regular gr…

astro-ph.CO2019

Detection and analysis of cluster-cluster filaments

Luis A. Pereyra, Mario A. Sgró, Manuel E. Merchán +2

In this work, we identify and analyse the properties of cluster-cluster filaments within a cosmological simulation assuming that they are structures connecting maxima of the densit…