output
20022026
most citedThe Gaia mission

7.1k citations

Showing 2024Show all

110 papers · 1 filter

astro-ph.GA202412 cited

Modelling chemical clocks -- Theoretical evidences of the space and time evolution of [s/alpha] in the Galactic disc with Gaia-ESO survey

Marta Molero, Laura Magrini, Marco Palla +6

Chemical clocks based on [s-process elements/alpha-elements] ratios are widely used to estimate ages of Galactic stellar populations. However, the [s/alpha] vs. age relations are n…

astro-ph.GA20246 cited

The JWST-NIRCam View of Sagittarius C. II. Evidence for Magnetically Dominated HII Regions in the CMZ

John Bally, Samuel Crowe, Rubén Fedriani +11

We present JWST-NIRCam narrow-band, 4.05 m Brackett- images of the Sgr C HII region, located in the Central Molecular Zone (CMZ) of the Galaxy. Unlike any HII region in the S…

astro-ph.EP20246 cited

Radii, masses, and transit-timing variations of the three-planet system orbiting the naked-eye star TOI-396

A. Bonfanti, I. Amateis, D. Gandolfi +38

TOI-396 is an F6V star () orbited by three transiting planets. The orbital periods of the two innermost planets are close to the 5:3 commensurability ( d…

astro-ph.SR20243 cited

Investigating the asymmetry of young stellar outflows: Combined MUSE-X-shooter study of the Th 28 jet

A. Murphy, E. T. Whelan, F. Bacciotti +7

Characterising stellar jet asymmetries is key to setting robust constraints on jet launching models and improving our understanding of the underlying mechanisms behind jet launchin…

astro-ph.IM20242 cited

The Survey of Surveys: machine learning for stellar parametrization

A. Turchi, E. Pancino, F. Rossi +6

We present a machine learning method to assign stellar parameters (temperature, surface gravity, metallicity) to the photometric data of large photometric surveys such as SDSS and…

astro-ph.EP20245 cited

The GAPS programme at TNG LXVI. A homogeneous search for Na i and its possible variability in ten gas giant exoplanets

D. Sicilia, L. Malavolta, G. Scandariato +18

The neutral sodium resonance doublet (Na i D) has been detected in the upper atmosphere of several close-in gas giants, through high-resolution transmission spectroscopy. We aim to…