Tadafumi Matsuno

Heidelberg University — Germany

Physics and Astronomy · Physical Sciences

16h-index1.1kcitations97works3.52yr avg
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Research Topics

Stellar, planetary, and galactic studies(76), Astronomy and Astrophysical Research(63), Astrophysics and Star Formation Studies(30), Astro and Planetary Science(13), Gamma-ray bursts and supernovae(12)

Publications95 total

Nucleochronology with HRMOS
Zenodo (CERN European Organization for Nuclear Research)·2026Open Access
Nucleochronology with HRMOS
Zenodo (CERN European Organization for Nuclear Research)·2026Open Access
HR-GO. II. Chemical Abundances of Low- <i>E</i> Retrograde Dynamically Tagged Groups: Revealing Thamnos as a Very Metal-poor Substructure
The Astrophysical Journal·2026Open Access
The Pristine survey
Springer Link (Chiba Institute of Technology)·2026
Variations in the Milky Way’s Stellar Mass Function at [Fe/H] &lt; −1
The Astrophysical Journal Letters·2026Open Access
Variations in the Milky Way's Stellar Mass Function at [Fe/H] &lt; -1
arXiv (Cornell University)·2026Open Access
HR-GO II: chemical abundances of low-$E$ retrograde dynamically-tagged-groups: Revealing Thamnos as a very metal-poor substructure
arXiv (Cornell University)·2026Open Access
HR-GO II: chemical abundances of low-$E$ retrograde dynamically-tagged-groups: Revealing Thamnos as a very metal-poor substructure
ArXiv.org·2026Open Access
The Pristine survey
Astronomy and Astrophysics·2026Open Access
The Pristine survey
Astronomy and Astrophysics·2026Open Access
The metal-poor tail of the APOGEE survey
Astronomy and Astrophysics·2025Open Access
A nearly pristine star from the Large Magellanic Cloud
ArXiv.org·2025· 1 citedOpen Access
Chemical Abundances of Seven Stars in the GD-1 Stream
The Astrophysical Journal Letters·2025Open Access
Improving MedDRA/J Coding Accuracy with a Fine-Tuned Text Embedding Model
Studies in health technology and informatics·2025Open Access
A Pristine-UNIONS view on the Galaxy: Kinematics of the distant spur feature of the Sagittarius stream traced by blue horizontal branch stars
Astronomy and Astrophysics·2025· 4 citedOpen Access
Chemical abundances of seven stars in the GD-1 stream
arXiv (Cornell University)·2025Open Access
Unevolved Li-rich stars at low metallicity: A possible formation pathway through novae
Springer Link (Chiba Institute of Technology)·2025
Chemical characterisation of small substructures in the local stellar halo
Astronomy and Astrophysics·2025· 2 citedOpen Access
Th/Eu abundance ratio of red giants in the Kepler field
Astronomy and Astrophysics·2025· 1 citedOpen Access
Unevolved Li-rich stars at low metallicity: A possible formation pathway through novae
Astronomy and Astrophysics·2025· 1 citedOpen Access
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Frequent Co-authors

Wako Aoki(20), A. Helmi(12), Takuma Suda(11), Else Starkenburg(11), Haining Li(10), Miho N. Ishigaki(10), Federico Sestito(10), Gang Zhao(9), Nicolas F. Martin(9), Anke Arentsen(9), Emma Dodd(8), Jingkun Zhao(7), Qianfan Xing(6), Satoshi Honda(6), Jianrong Shi(6), T. Ruiz-Lara(6), E. Balbinot(6), Akshara Viswanathan(6), Kim A. Venn(6), Sara Vitali(6)