activity
20152022
most citedThe Uchuu Simulations: Data Release 1 and Dark Matter Halo Concentrations

273 citations · 437 across the 11 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2022

Anisotropic infall in the outskirst of clusters

Juan Manuel Salerno, Hernán Muriel, Valeria Coenda +4

We analyse the connection between the star formation quenching of galaxies and their location in theoutskirts of clusters in the redshift range by estimating the fraction…

astro-ph.CO2021★ 11 cited

Tracking the orbit of unresolved subhalos for semi-analytic models

Facundo M. Delfino, Claudia G. Scoccola, Sofia A. Cora +2

We present a model to track the orbital evolution of "unresolved subhaloes" (USHs) in cosmological simulations. USHs are subhaloes that are no longer distinguished by halo finders…

astro-ph.GA2020★ 20 cited

ROGER: Reconstructing Orbits of Galaxies in Extreme Regions using machine learning techniques

Martín de los Rios, Héctor Julián Martínez, Valeria Coenda +4

We present the ROGER (Reconstructing Orbits of Galaxies in Extreme Regions) code, which uses three different machine learning techniques to classify galaxies in, and around, cluste…

astro-ph.GA2020★ 3 cited

Associations of dwarf galaxies in a CDM Universe

C. Y. Yaryura, M. G. Abadi, S. Gottlober +6

Associations of dwarf galaxies are loose systems composed exclusively of dwarf galaxies. These systems were identified in the Local Volume for the first time more than thirty years…

astro-ph.GA2020★ 26 cited

Investigating The Growing Population of Massive Quiescent Galaxies at Cosmic Noon

Sydney Sherman, Shardha Jogee, Jonathan Florez +10

We explore the buildup of quiescent galaxies using a sample of 28,469 massive (M) galaxies at redshifts , drawn from a 17.5 deg area (0.…

astro-ph.CO2020★ 273 cited

The Uchuu Simulations: Data Release 1 and Dark Matter Halo Concentrations

Tomoaki Ishiyama, Francisco Prada, Anatoly A. Klypin +11

We introduce the Uchuu suite of large high-resolution cosmological -body simulations. The largest simulation, named Uchuu, consists of 2.1 trillion () dark matter parti…

astro-ph.GA2019

Siblings, friends and acquaintances: Testing galaxy association methods

J. P. Caso, C. A. Vega-Martínez

In order to constraint the limitations of association methods applied to galaxy surveys, we analysed the catalogue of halos at of a cosmological simulation, trying to reprodu…

astro-ph.GA2019★ 21 cited

[OII] emitters in MultiDark-Galaxies and DEEP2

G. Favole, V. Gonzalez-Perez, A. Orsi +13

We use three semi-analytic models (SAMs) of galaxy formation and evolution, run on the same 1Gpc MultiDark Planck2 cosmological simulation, to investigate the properties of…

astro-ph.GA2018★ 29 cited

Semi-analytic galaxies -- III. The impact of supernova feedback on the mass-metallicity relation

Florencia Collacchioni, Sofía A. Cora, Claudia D. P. Lagos +1

We use the semi-analytic model (SAM) of galaxy formation and evolution SAG coupled with the MULTIDARK simulation MDPL2 to study the evolution of the stellar mass-gas metallicity re…

astro-ph.GA2018★ 22 cited

Cosmic CARNage II: the evolution of the galaxy stellar mass function in observations and galaxy formation models

Rachel Asquith, Frazer R. Pearce, Omar Almaini +24

We present a comparison of the observed evolving galaxy stellar mass functions with the predictions of eight semi-analytic models and one halo occupation distribution model. While…

astro-ph.GA2018★ 32 cited

Semi-Analytic Galaxies - II. Revealing the role of environmental and mass quenching in galaxy formation

Sofía A. Cora, Tomás Hough, Cristian A. Vega-Martínez +1

We use the semi-analytic model of galaxy formation SAG to study the relevance of mass and environmental quenching on satellite galaxies. We find that environmental processes domina…

astro-ph.GA2015

nIFTy Cosmology: Comparison of Galaxy Formation Models

Alexander Knebe, Frazer R. Pearce, Peter A. Thomas +33

We present a comparison of 14 galaxy formation models: 12 different semi-analytical models and 2 halo-occupation distribution models for galaxy formation based upon the same cosmol…