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20052026
most citedThe Gaia-ESO Survey: the Galactic Thick to Thin Disc transition

241 citations · 5.5k across the 134 of their papers we have counts for

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Showing astro-ph.GAShow all

35 papers · 1 filter

astro-ph.GA2025★ 5 cited

Probing the origins. I. Generalised Additive Model inference of birth radii for Milky Way stars in the solar vicinity

M. L. L. Dantas, R. Smiljanic, R. S. de Souza +2

We employ a Generalised Additive Model (GAM) to address the limitations inherent in radial metallicity gradients predicted by chemical evolution models, thereby facilitating the es…

astro-ph.GA2024★ 129 cited

Discovery of a dormant 33 solar-mass black hole in pre-release Gaia astrometry

Gaia Collaboration, P. Panuzzo, T. Mazeh +412

Gravitational waves from black-hole merging events have revealed a population of extra-galactic BHs residing in short-period binaries with masses that are higher than expected base…

astro-ph.GA2023★ 7 cited

Gaia Focused Product Release: A catalogue of sources around quasars to search for strongly lensed quasars

Gaia Collaboration, A. Krone-Martins, C. Ducourant +398

Context. Strongly lensed quasars are fundamental sources for cosmology. The Gaia space mission covers the entire sky with the unprecedented resolution of " in the optical, ma…

astro-ph.GA2023★ 14 cited

Exploring the chemodynamics of metal-poor stellar populations

André Rodrigo da Silva, Rodolfo Smiljanic

Metal-poor stars are key for studying the formation and evolution of the Galaxy. Evidence of the early mergers that built up the Galaxy remains in the distributions of abundances,…

astro-ph.GA2023★ 22 cited

Chronology of the chemical enrichment of the old Galactic stellar populations

Riano E. Giribaldi, Rodolfo Smiljanic

The Milky Way accreted several smaller satellite galaxies in its history. These mergers added stars and gas to the Galaxy and affected the properties of the pre-existing stellar po…

astro-ph.GA2022★ 15 cited

The Gaia-ESO Survey: Old super-metal-rich visitors from the inner Galaxy

M. L. L. Dantas, R. Smiljanic, R. Boesso +12

We report the identification of a set of old super metal-rich dwarf stars with orbits of low eccentricity that reach a maximum height from the Galactic plane between ~0.5-1.5 kpc.…