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- 2020
- The HR 1614 moving group is not a dissolving cluster (
- Modelling the chemical evolution of Zr, La, Ce, and Eu in the Galactic discs and bulge (
- The Gaia -ESO Survey : Galactic evolution of lithium at high metallicity (
- Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars : VII. Lithium (
- Constraining churning and blurring in the Milky Way using large spectroscopic surveys - An exploratory study (
- The Gaia -ESO survey : The non-universality of the age-chemical-clocks-metallicity relations in the Galactic disc (
- Fluorine in the solar neighbourhood : Modelling the Galactic thick and thin discs (
- 2019
- The GALAH survey : An abundance, age, and kinematic inventory of the solar neighbourhood made with TGAS (
- Kinematics with GAIA DR2 : The force of a dwarf (
- The COMBS survey – I. Chemical origins of metal-poor stars in the Galactic bulge (