activity
20102023
most citedGalactic conformity measured in semi-analytic models

27 citations · 67 across the 6 of their papers we have counts for

collaborators

6 papers

physics.ins-det2023★ 1 cited

A Compact Dication Source for Ba Tagging and Heavy Metal Ion Sensor Development

K. E. Navarro, B. J. P. Jones, J. Baeza-Rubio +107

We present a tunable metal ion beam that delivers controllable ion currents in the picoamp range for testing of dry-phase ion sensors. Ion beams are formed by sequential atomic eva…

astro-ph.IM2018★ 1 cited

Galaxy detection and identification using deep learning and data augmentation

Roberto E. González, Roberto P. Muñoz, Cristian A. Hernández

We present a method for automatic detection and classification of galaxies which includes a novel data-augmentation procedure to make trained models more robust against the data ta…

astro-ph.GA2017★ 6 cited

Stellar Populations in a semi-analytic model I: bulges of Milky Way-like galaxies

I. D. Gargiulo, S. A. Cora, C. A. Vega-Martínez +5

We study the stellar populations of bulges of Milky Way-like (MW-like) galaxies with the aim of identifying the physical processes involved in the formation of the bulge of our Gal…

astro-ph.GA2017★ 27 cited

Galactic conformity measured in semi-analytic models

Ivan Lacerna, Sergio Contreras, Roberto E. González +2

We study the correlation between the specific star formation rate of central galaxies and neighbour galaxies, also known as 'galactic conformity', out to 20 Mpc/h using three semi-…

astro-ph.CO2014★ 23 cited

The origin of spin in galaxies: clues from simulations of atomic cooling halos

Joaquin Prieto, Raul Jimenez, Zoltán Haiman +1

In order to elucidate the origin of spin in both dark matter and baryons in galaxies, we have performed hydrodynamical simulations from cosmological initial conditions. We study at…

astro-ph.CO2010★ 9 cited

Clustering and descendants of MUSYC galaxies at z<1.5

Nelson Padilla, Daniel Christlein, Eric Gawiser +3

We measure the evolution of galaxy clustering out to a redshift of z~1.5 using data from two MUSYC fields, the Extended Hubble Deep Field South (EHDF-S) and the Extended Chandra De…