output
20152026
most citedThe Gaia mission

7.1k citations

31 papers

astro-ph.SR2026

Discovery of sulfur oxides in the ejecta of a B[e] supergiant

C. Bordiu, J. Ricardo Rizzo, D. Navarro-Almaida +12

B[e] supergiants represent a rare class of luminous, evolved massive stars surrounded by dusty circumstellar disks. Since their intense UV fields were long thought to sterilize the…

astro-ph.EP2026

ExoDNN: Boosting exoplanet detection with artificial intelligence. Application to Gaia Data Release 3

A. Abreu, J. Lillo-Box, A. M. Perez-Garcia +3

We combine Gaia Data Release 3 and artificial intelligence to enhance the current statistics of substellar companions, particularly within regions of the orbital period vs. mass pa…

astro-ph.GA2025★ 1 cited

GLACE survey: OSIRIS/GTC multi-object spectroscopy of the rich galaxy cluster ZwCl 0024.0+1652 at z~0.4. III. The mass-SFR relation and the quenching of cluster galaxies

Simon B. De Daniloff, Ángel Bongiovanni, Miguel Sánchez-Portal +21

Galaxy clusters are among the largest and densest structures in the Universe. Their high density generally increases the suppression of star formation, known as quenching, altering…

astro-ph.GA2025★ 1 cited

MeerKAT discovery of 164 compact radio rings toward the Galactic Plane

C. Bordiu, F. Bufano, G. Umana +14

We report the discovery of 164 compact (radius < 1 arcmin) radio rings using MeerKAT 1.3 GHz data from the SARAO MeerKAT Galactic Plane Survey (l=2-60deg, 252-358deg, |b|<1.5deg) a…

astro-ph.SR2025★ 1 cited

Millimetre continuum from LBV stars and their environs. NIKA2 observations and Virtual Observatory data

J. R. Rizzo, C. Bordiu, A. Ritacco

Multi-wavelength studies of their circumstellar environments around LBVs are essential to quantify their feedback at Galactic scales. Dominant emission mechanisms at millimetre wav…

astro-ph.SR2024

Substellar candidates at the earliest stages: the SUCANES database

A. M. Pérez-García, N. Huélamo, A. García-López +11

Brown dwarfs are the bridge between low-mass stars and giant planets. One way of shedding light on their dominant formation mechanism is to study them at the earliest stages of the…