activity
20082025
most citedChemical Evolution of R-process Elements in Stars (CERES). I. Stellar parameters and chemical abundances from Na to Zr

27 citations · 116 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2025★ 4 cited

Unveiling the nature of HE 0107-5240

E. Caffau, M. Steffen, P. Molaro +27

The vast majority of the most iron-poor stars in the Galaxy exhibit a strong carbon enhancement, with C/H ratios only about two orders of magnitude below solar. This unusual chemic…

astro-ph.GA2025★ 5 cited

MINCE III. Detailed chemical analysis of the UVES sample

F. Lucertini, L. Sbordone, E. Caffau +14

Context. The MINCE (Measuring at Intermediate Metallicity Neutron-Capture Elements) project aims to provide high quality neutron-capture abundances measurements in several hundred…

astro-ph.GA2024★ 11 cited

SDSS J102915.14+172927.9: Revisiting the chemical pattern

E. Caffau, P. Bonifacio, L. Monaco +7

Context: The small- to intermediate-mass (), most metal-poor stars that formed in the infancy of the Universe are still shining today in the sky. They are very rare…

astro-ph.SR2024★ 5 cited

High speed stars: III. Detailed abundances and binary nature of the extreme speed star GHS143

E. Caffau, P. Bonifacio L. Monaco, L. Sbordone +7

The Gaia satellite has provided the community with three releases containing astrometrical and photometric data as well as by products, such as stellar parameters and variability i…

astro-ph.GA2024★ 14 cited

High-speed stars. II. An unbound star, young stars, bulge metal-poor stars, and Aurora candidates

P. Bonifacio, E. Caffau, L. Monaco +6

The data from the Gaia satellite led us to revise our conception of the Galaxy structure and history. Hitherto unknown components have been discovered and a deep re-thinking of wha…

astro-ph.SR2022★ 22 cited

The Gaia-ESO Survey: Lithium measurements and new curves of growth

E. Franciosini, S. Randich, P. de Laverny +37

The Gaia-ESO Survey (GES) is a large public spectroscopic survey that was carried out using the multi-object FLAMES spectrograph at the Very Large Telescope. The survey provides ac…