The contribution of UVES@VLT to the new era of QSO absorption line studies
Valentina D'Odorico, Miroslava Dessauges-Zavadsky

TL;DR
This paper reviews the significant contributions of the UVES high-resolution spectrograph on the VLT to advancing quasar absorption line research, highlighting key results and developments in the field.
Contribution
It provides a comprehensive overview of how UVES has enhanced QSO absorption line studies, emphasizing new insights gained from high-resolution spectroscopy.
Findings
UVES enabled precise measurements of absorption lines.
The instrument contributed to understanding the intergalactic medium.
Significant improvements in spectral resolution and data quality.
Abstract
We briefly review the main results obtained in the field of QSO absorption line studies with the UVES high resolution spectrograph mounted on the Kueyen unit of the ESO Very Large Telescope (Paranal, Chile).
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Taxonomy
TopicsAstronomy and Astrophysical Research · Stellar, planetary, and galactic studies · Gamma-ray bursts and supernovae
