activity
19962026
most citedThe Slope of the Cluster Elliptical Red Sequence: A Probe of Cluster Evolution

181 citations · 1.2k across the 26 of their papers we have counts for

collaborators

28 papers

astro-ph.GA2026

Sub-kiloparsec Test of the Kennicutt-Schmidt Relation in a Strongly Lensed Dusty Star-Forming Galaxy at z~2.78

C. Cornil-Baïotto, J. Molina, G. Mahler +9

[abridged] Star formation is a key process driving galaxy evolution, but understanding how it proceeds within the interstellar medium (ISM) requires resolving cold molecular gas an…

astro-ph.GA2022★ 12 cited

Metal-THINGS: The association and optical characterization of SNRs with HI holes in NGC 6946

M. A. Lara-Lopez, L. S. Pilyugin, J. Zaragoza-Cardiel +9

NGC~6946, also known as the `Fireworks' galaxy, is an unusual galaxy that hosts a total of 225 supernova remnant (SNR) candidates, including 147 optically identified with high [SII…

gr-qc2020★ 18 cited

Toward the Gravitational Redshift Detection in NGC 4258 and the Estimation of its Black Hole Mass-to-Distance Ratio

Ulises Nucamendi, Alfredo Herrera-Aguilar, Raul Lizardo-Castro +1

We construct from first principles a general relativistic approach to study Schwarzschild black hole (BH) rotation curves and estimate the mass-to-distance ratio of the active gala…

astro-ph.GA2020★ 17 cited

Metal-THINGS: On the metallicity and ionization of ULX sources in NGC 925

Maritza A. Lara-López, Igor A. Zinchenko, Leonid S. Pilyugin +13

We present an analysis of the optical properties of three Ultra Luminous X-ray (ULX) sources identified in NGC 925. We use Integral field unit data from the George Mitchel spectrog…

astro-ph.HE2019★ 5 cited

TOROS Optical follow-up of the Advanced LIGO-VIRGO O2 second observational campaign

Rodolfo Artola, Martin Beroiz, Juan Cabral +48

We present the results of the optical follow-up, conducted by the TOROS collaboration, of gravitational wave events detected during the Advanced LIGO-Virgo second observing run (No…

astro-ph.GA2018★ 13 cited

The `Cosmic Seagull': a highly magnified disk-like galaxy at z~2.8 behind the Bullet Cluster

V. Motta, E. Ibar, T. Verdugo +8

We present Atacama Large Millimeter/submillimeter Array measurements of the `Cosmic Seagull', a strongly magnified galaxy at z=2.7779 behind the Bullet Cluster. We report CO(3-2) a…