activity
20242026
collaborators

9 papers

astro-ph.GA2026

A homogeneous three-dimensional view of Molecular Cloud kinematics out to 2.5 kpc. Using Young Stellar Objects and Open Clusters as complementary tracers

Xabier Pérez-Couto, Santiago Torres, Nuria Miret-Roig +4

Understanding the large-scale dynamics of molecular clouds (MCs) is crucial for constraining the processes that govern star formation and the structure and evolution of the Galaxy.…

astro-ph.SR2026

Detection of hot subdwarf binaries and sdB stars using machine learning methods and a large sample of Gaia XP spectra

M. Ambrosch, C. Viscasillas Vázquez, E. Solano +10

Hot subdwarfs (hot sds) are compact, evolved stars near the Extreme Horizontal Branch (EHB) and are key to understanding stellar evolution and the ultraviolet excess in galaxies. W…

astro-ph.SR2025

Finding White Dwarfs' Hidden Companions using an Unsupervised Machine Learning Technique

Xabier Pérez-Couto, Minia Manteiga, Eva Villaver

White dwarfs (WD) with main-sequence (MS) companions are crucial probes of stellar evolution. However, due to the significant difference in their luminosities, the WD is often outs…

astro-ph.IM2025

Disentangling stellar atmospheric parameters in astronomical spectra using Generative Adversarial Neural Networks

Minia Manteiga, Raúl Santoveña, Marco A. Álvarez +4

A method based on Generative Adversaria! Networks (GANs) is developed for disentangling the physical (effective temperature and gravity) and chemical (metallicity, overabundance of…

astro-ph.IM2024

A method based on Generative Adversarial Networks for disentangling physical and chemical properties of stars in astronomical spectra

Raúl Santoveña, Carlos Dafonte, Minia Manteiga

Data compression techniques focused on information preservation have become essential in the modern era of big data. In this work, an encoder-decoder architecture has been designed…

astro-ph.SR2024

Identifying new high-confidence polluted white dwarf candidates using Gaia XP spectra and Self-Organizing Maps

Xabier Pérez-Couto, Lara Pallas-Quintela, Minia Manteiga +2

The identification of new white dwarfs (WDs) polluted with heavy elements is important since they provide a valuable tool for inferring chemical properties of putative planetary sy…