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Principal component analysis on chemical abundances spaces
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METALLICITY EVOLUTION OF DAMPED Lyα SYSTEMS OUT TOz∼ 5
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Non-LTE line formation of Fe in late-type stars – I. Standard stars with 1D and 〈3D〉 model atmospheres
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Both accurate and precisegf-values for Fe II lines
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Coincident, 100 kpc scale damped Lyα absorption towards a binary QSO: how large are galaxies at z ∼ 3?
Sara L. Ellison, Joseph F. Hennawi, Crystal L. Martin and Jesper Sommer-Larsen Monthly Notices of the Royal Astronomical Society 378(3) 801 (2007) https://doi.org/10.1111/j.1365-2966.2007.11847.x
Sulphur abundances from the S i near-infrared triplet at 1045 nm
Probing the Interstellar Medium near Star‐forming Regions with Gamma‐Ray Burst Afterglow Spectroscopy: Gas, Metals, and Dust
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The Chemical Evolution of High‐zGalaxies from the Relative Abundances of N, Si, S, and Fe in Damped Lyα Systems
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