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20102026
most citedESPRESSO@VLT -- On-sky performance and first results

537 citations · 5.1k across the 108 of their papers we have counts for

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astro-ph.SR2026

Astro+ database. I. Description and first results

K. Rübke, A. Marco, I. Negueruela +4

The vast amounts of spectroscopic data for massive stars provided by previous and existing instruments on ground-based and space-based telescopes have saturated our capability to p…

astro-ph.SR2026

The CARMENES search for exoplanets around M dwarfs. A homogeneous catalogue of projected rotational velocities accounting for limb-darkening

R. Varas, G. Morello, M. Zechmeister +18

Stellar rotation is closely linked to both age and magnetic activity. Through gyrochronology, it provides a means to estimate stellar ages and trace the evolution of planetary syst…

astro-ph.SR2025

A neural network approach to determining photometric metallicities of M-type dwarf stars

C. Duque-Arribas, H. M. Tabernero, D. Montes +2

M dwarfs are the most abundant stars in the Galaxy and serve as key targets for stellar and exoplanetary studies. It is particularly challenging to determine their metallicities be…

astro-ph.SR2024

CARMENES input catalogue of M dwarfs VIII. Kinematics in the solar neighbourhood

M. Cortés-Contreras, J. A. Caballero, D. Montes +15

Aims. Our goals are to characterise the kinematic properties and to identify young and old stars among the M dwarfs of the CARMENES input catalogue. Methods. We compiled the spectr…

astro-ph.SR2024

The CARMENES search for exoplanets around M dwarfs: Magnesium and silicon abundances of K7-M5.5 stars

H. M. Tabernero, Y. Shan, J. A. Caballero +13

We present the abundances of magnesium (Mg) and silicon (Si) for 314 dwarf stars with spectral types in the interval K7.0-M5.5 (Teff range ~4200-3050 K) observed with the CARMENES…

astro-ph.SR2024★ 14 cited

Using autoencoders and deep transfer learning to determine the stellar parameters of 286 CARMENES M dwarfs

P. Mas-Buitrago, A. González-Marcos, E. Solano +9

Deep learning (DL) techniques are a promising approach among the set of methods used in the ever-challenging determination of stellar parameters in M dwarfs. In this context, trans…