V. Grisoni

Trieste Astronomical Observatory — Italy

Physics and Astronomy · Physical Sciences

17h-index882citations42works0.52yr avg
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Research Topics

Stellar, planetary, and galactic studies(35), Astronomy and Astrophysical Research(24), Astrophysics and Star Formation Studies(22), Astro and Planetary Science(7), Gamma-ray bursts and supernovae(5)

Publications42 total

Asteroseismic ages for 17,000 stars in <i>Kepler</i> , K2 and TESS
Monthly Notices of the Royal Astronomical Society·2026Open Access
Asteroseismic ages for 17,000 stars in Kepler, K2 and TESS
arXiv (Cornell University)·2026Open Access
Asteroseismic ages for 17,000 stars in Kepler, K2 and TESS
ArXiv.org·2026Open Access
Fluorine evolution in the Galactic halo
Astronomy and Astrophysics·2025Open Access
Fluorine Evolution in the Galactic Halo
arXiv (Cornell University)·2025Open Access
Tracing the Milky Way: calibrating chemical ages with high-precision <i>Kepler</i> data
Monthly Notices of the Royal Astronomical Society·2025· 3 citedOpen Access
Tracing the Milky Way: Calibrating chemical ages with high-precision Kepler data
arXiv (Cornell University)·2025Open Access
Fluorine Abundances in Local Stellar Populations
The Astronomical Journal·2024· 1 citedOpen Access
K2 results for “young” <i>α</i>-rich stars in the Galaxy
Astronomy and Astrophysics·2023· 19 citedOpen Access
K2 results for "young" $α$-rich stars in the Galaxy
arXiv (Cornell University)·2023Open Access
Asteroseismic age estimate of the open cluster NGC 6866 using <i>Kepler</i> and <i>Gaia</i>
Astronomy and Astrophysics·2023· 13 citedOpen Access
An asteroseismic age estimate of the open cluster NGC 6866 using Kepler and Gaia
arXiv (Cornell University)·2023Open Access
The evolution of the Milky Way’s thin disc radial metallicity gradient with K2 asteroseismic ages
Monthly Notices of the Royal Astronomical Society·2023· 24 citedOpen Access
The evolution of the Milky Way's thin disc radial metallicity gradient with K2 asteroseismic ages
arXiv (Cornell University)·2023Open Access
Time evolution of Ce as traced by APOGEE using giant stars observed with the <i>Kepler</i>, TESS and K2 missions
Astronomy and Astrophysics·2023· 8 citedOpen Access
Time evolution of Ce as traced by APOGEE using giant stars observed with the Kepler, TESS and K2 missions
arXiv (Cornell University)·2023· 2 citedOpen Access
The cerium content of the Milky Way as revealed by <i>Gaia</i> DR3 GSP-Spec abundances
Astronomy and Astrophysics·2022· 17 citedOpen Access
The cerium content of the Milky Way as revealed by Gaia DR3 GSP-Spec abundances
arXiv (Cornell University)·2022Open Access
Impact of very massive stars on the chemical evolution of extremely metal-poor galaxies
Astronomy and Astrophysics·2022· 24 citedOpen Access
Nitrogen evolution in the halo, thick disc, thin disc, and bulge of the Galaxy
Monthly Notices of the Royal Astronomical Society·2021· 12 citedOpen Access
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Frequent Co-authors

F. Matteuccí(22), G. Casali(15), E. Spitoni(13), E. Willett(13), C. Chiappini(11), Amalie Stokholm(11), A. Miglio(10), D. Romano(8), M. Tailo(8), G. Cescutti(7), J. Montalbán(7), L. Magrini(6), Y. Elsworth(6), B. Mosser(6), K. Brogaard(6), M. Matteuzzi(6), P. de Laverny(5), S. Khan(5), A. Recio–Blanco(4), C. C. Worley(4)