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Nature of the Absorbing Gas associated with a Galaxy Group at z~0.4, , , , , , , , and . (2016)cite arxiv:1609.07389Comment: Accepted for publication in MNRAS; 14 pages, 12 figures.Early metal enrichment of gas-rich galaxies at z~5, , , , , , and . (2017)cite arxiv:1710.03315Comment: 15 pages, 14 figures, accepted for publication in MNRAS.A SINFONI Integral Field Spectroscopy Survey for Galaxy Counterparts to Damped Lyman-alpha Systems - VI. Metallicity and Geometry as Gas Flow Probes, , , , , , , , , and . (2016)cite arxiv:1601.02796Comment: 16 pages, 8 figures, accepted for publication in MNRAS.Atomic Data Revisions for Transitions Relevant to Observations of Interstellar, Circumgalactic, and Intergalactic Matter, , , , and . (2017)cite arxiv:1701.04847Comment: Submitted to the Astrophysical Journal Supplement Series; includes 1 machine-readable table.Element Abundances at High-redshift: Magellan MIKE Observations of sub-Damped Lyman-alpha Absorbers at 1.7 < z <2.4, , , , , , and . (2013)cite arxiv:1307.7103Comment: Accepted for publication in the Monthly Notices of The Royal Astronomical Society.Exploring the dust content of SDSS DR7 damped Lyman alpha systems at 2.15$z_ab&lt; $5.2, , , , and . (2011)cite arxiv:1109.4225Comment: 12 pages, 9 figures. To appear in MNRAS.A Super-Damped Lyman-alpha QSO Absorber at z=2.2, , , , , , and . (2012)cite arxiv:1202.0882 Comment: Revised version submitted to the Astrophysical Journal including responses to the referee report. Original version submitted on Dec. 10, 2011.Galaxies with Background QSOs, I: A Search for Strong Galactic H-alpha Lines, , , , , , , , , and 5 other author(s). (2012)cite arxiv:1204.5786.A study of the circum-galactic medium at z ~ 0.6 using DLA-galaxies, , , , , , , and . (2016)cite arxiv:1609.03843Comment: MNRAS accepted.Atomic data for Zn II - Improving Spectral Diagnostics of Chemical Evolution in High-redshift Galaxies, , , , , and . (2015)cite arxiv:1504.01667Comment: accepted The Astrophysical Journal.