Lund Observatory - Has been reorganised
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- 2024
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Mark
EDGE – Dark matter or astrophysics? Breaking dark matter heating degeneracies with H I rotation in faint dwarf galaxies
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- Contribution to journal › Article
- 2023
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Mark
Anatomy of rocky planets formed by rapid pebble accretion : II. Differentiation by accretion energy and thermal blanketing
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- Contribution to journal › Article
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Mark
Anatomy of rocky planets formed by rapid pebble accretion : III. Partitioning of volatiles between planetary core, mantle, and atmosphere
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- Contribution to journal › Article
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Mark
Anatomy of rocky planets formed by rapid pebble accretion : I. How icy pebbles determine the core fraction and FeO contents
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- Contribution to journal › Article
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Mark
Detailed α abundance trends in the inner Galactic bulge
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- Contribution to journal › Article
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The ESSnuSB Design Study: Overview and Future Prospects
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- Contribution to journal › Article
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Mark
The Gaia-ESO Survey : Preparing the ground for 4MOST and WEAVE galactic surveys: Chemical evolution of lithium with machine learning
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- Contribution to journal › Article
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Mark
Chrono-chemodynamical analysis of the globular cluster NGC 6355 : Looking for the fundamental bricks of the Bulge
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- Contribution to journal › Article
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Making hot Jupiters in stellar clusters: The importance of binary exchange
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- Contribution to journal › Article
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Mark
The chemical characterization of halo substructure in the Milky Way based on APOGEE
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- Contribution to journal › Article
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Mark
The Mantis network : A standard grid of templates and masks for cross-correlation analyses of ultra-hot Jupiter transmission spectra
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- Contribution to journal › Article
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The Gaia -ESO survey : Mapping the shape and evolution of the radial abundance gradients with open clusters
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- Contribution to journal › Article
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The Gaia -ESO Survey : Old super-metal-rich visitors from the inner Galaxy
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- Contribution to journal › Article
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Mark
Stellar ages, masses, extinctions, and orbital parameters based on spectroscopic parameters of Gaia DR3
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- Contribution to journal › Article
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Kinematic analysis of the Large Magellanic Cloud using Gaia DR3
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- Contribution to journal › Article