activity
20242026
most citedDisentangling the origin of chemical differences using GHOST

11 citations · 20 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2026

A very rapidly rotating white dwarf in nova YZ Reticuli

G. J. M. Luna, N. Rawat, R. Angeloni +4

YZ Ret (Nova Reticuli 2020) is the first VY Scl-type nova-like variable observed to undergo a classical nova eruption. Following the outburst, timing analysis of 20-s cadence TESS…

astro-ph.SR2026★ 1 cited

A search for new symbiotic stars in the Milky Way: Using machine learning techniques applied to photometric databases

V. Contreras Rojas, M. Jaque Arancibia, C. E. Ferreira Lopes +8

Symbiotic stars (SySts) are interacting binaries composed of a red giant transferring material to a hot compact star, typically a white dwarf. Although only about 300 systems are c…

astro-ph.SR2025

Astrophotometric search for massive stars in the Milky way. Confronting Random Forest predictions with available spectroscopy

N. Monsalves, A. Bayo, M. Jaque Arancibia +4

Massive stars play a significant role in different branches of astronomy, from shaping the processes of star and planet formation to influencing the evolution and chemical enrichme…

astro-ph.IM2025

A First Quantitative Characterization of Colombian Night Sky Through All-Sky Photometry

J. P. Uchima-Tamayo, R. Angeloni, M. Jaque Arancibia +2

Light pollution, a rapidly escalating anthropogenic phenomenon driven by the excessive and often inefficient use of artificial lighting, has profound implications for astronomy, ec…

astro-ph.IM2024★ 8 cited

Application of Convolutional Neural Networks to time domain astrophysics. 2D image analysis of OGLE light curves

N. Monsalves, M. Jaque Arancibia, A. Bayo +4

In recent years the amount of publicly available astronomical data has increased exponentially, with a remarkable example being large scale multiepoch photometric surveys. This wea…

astro-ph.SR2024★ 11 cited

Disentangling the origin of chemical differences using GHOST

C. Saffe, P. Miquelarena, J. Alacoria +8

Aims. We explore different scenarios to explain the chemical difference found in the remarkable giant-giant binary system HD 138202 + CD-30 12303. For the first time, we suggest ho…