activity
20042025
most citedSignature of persistent metallic domains in FORC measurements of the VO metal-insulator transition

111 citations · 246 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.GA2025

The VVVX quest for satellites around the Circinus galaxy

L. D. Baravalle, A. L. O'Mill, M. V. Alonso +10

The Circinus galaxy is the nearest type-2 Seyfert galaxy, which is at a distance of 4.2 Mpc. Its environment is challenging to explore because it is located at low Galactic latitud…

astro-ph.GA2025

The VVV near-IR galaxy catalogue of the southern Galactic disc

M. V. Alonso, L. D. Baravalle, J. L. Nilo Castellón +16

The distribution of galaxies in the Zone of Avoidance (ZoA) is incomplete due to the presence of our own Galaxy. Our research focused on the identification and characterisation of…

astro-ph.GA2025★ 1 cited

Multi-Wavelength characterization of VVVX open clusters

C. O. Obasi, E. R. Garro, J. G. Fernández-Trincado +4

Context. Large-scale surveys across wavelengths, aided by machine learning, have improved the detection of old open clusters in high-extinction Milky Way regions. Aims. We aim to c…

astro-ph.GA2024

VVVX survey dusts off a new intermediate-age star cluster in the Milky Way disk

E. R. Garro, D. Minniti, J. Alonso-García +5

Our primary long-term objective is to seek out additional star clusters in the poorly studied regions of the MW. The aim of this pursuit is to finalize the MG's globular and open c…

astro-ph.GA2022★ 9 cited

The globular cluster system of the nearest Seyfert II galaxy Circinus

C. Obasi, M. Gómez, D. Minniti +7

Context. The globular cluster (GC) system of Circinus galaxy has not been probed previously partly because of the location of the galaxy at - 3.8 Galactic latitude which su…

astro-ph.SR2022

High-contrast imaging of HD 29992 and HD 196385 with GPI

Luciano H. García, R. Petrucci, E. Jofré +1

Based on high contrast images obtained with the Gemini Planet Imager (GPI), we report the discovery of two point-like sources at angular separations of and $ρ\sim0.80…