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Lind, K.
name
Lind, K.
Lind, Karin
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karin.lind@physics.uu.se
klind@ast.cam.ac.uk
klind@mpa-garching.mpg.de
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K.
Karin
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of
The Gaia-ESO Survey: the Galactic thick to thin disc transition
The Gaia-ESO Survey: The analysis of high-resolution UVES spectra of FGK-type stars
The Gaia-ESO Survey: Empirical determination of the precision of stellar radial velocities and projected rotation velocities
Atomic diffusion and mixing in old stars
The Gaia-ESO Survey: Abundance ratios in the inner-disk open clusters Trumpler 20, NGC 4815, NGC 6705
The Gaia-ESO Survey: Kinematic structure in the Gamma Velorum cluster
Gaia FGK benchmark stars: Metallicity
Gaia-ESO Survey: Empirical classification of VLT/Giraffe stellar spectra in the wavelength range 6440-6810 Å in the γ Velorum cluster, and calibration of spectral indices
Departures from LTE for neutral Li in late-type stars
Non-LTE calculations for neutral Na in late-type stars using improved atomic data
The influence of electron collisions on non-LTE Li line formation in stellar atmospheres
The lithium isotopic ratio in very metal-poor stars
The Gaia-ESO Survey: processing FLAMES-UVES spectra
The elemental composition of the Sun
Signatures of intrinsic Li depletion and Li-Na anti-correlation in the metal-poor globular cluster NGC 6397
Gaia FGK benchmark stars: abundances of α and iron-peak elements
The Gaia-ESO Survey: Spectroscopic-asteroseismic analysis of K2 stars in Gaia-ESO
Automatic line selection for abundance determinations in large stellar spectroscopic surveys
The double sub-giant branch of NGC 6656 (M 22): a chemical characterization
The Gaia-ESO Survey: radial metallicity gradients and age-metallicity relation of stars in the Milky Way disk
Mg line formation in late-type stellar atmospheres
The Gaia-ESO Survey: A globular cluster escapee in the Galactic halo
The Gaia-ESO Survey: Sodium and aluminium abundances in giants and dwarfs
Spectral diagnostics of late-type stars: Non-LTE and <3D> approach
Lithium depletion in solar-like stars: no planet connection
Tracing the evolution of NGC 6397 through the chemical composition of its stellar populations
LTE or non-LTE, that is the question
Gaia-ESO Survey: Properties of the intermediate age open cluster NGC 4815
Gaia-ESO Survey: Analysis of pre-main sequence stellar spectra
The Gaia-ESO Survey: characterisation of the [ α/Fe] sequences in the Milky Way discs
The Gaia-ESO Survey: New constraints on the Galactic disc velocity dispersion and its chemical dependencies
The Gaia-ESO Survey: Separating disk chemical substructures with cluster models
Gaia FGK benchmark stars: new candidates at low metallicities
The Gaia-ESO Survey: Churning through the Milky Way
The Gaia-ESO Survey: Lithium enrichment histories of the Galactic thick and thin disc
Effective temperature determinations of late-type stars based on 3D non-LTE Balmer line formation
Exploring the production and depletion of lithium in the Milky Way stellar disk
The Gaia-ESO Survey: properties of newly discovered Li-rich giants
Carbon and oxygen in metal-poor halo stars
Ca line formation in late-type stellar atmospheres
The GALAH survey: An abundance, age, and kinematic inventory of the solar neighbourhood made with TGAS
Non-LTE analysis of K I in late-type stars
The LUMBA UVES stellar parameter pipeline
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