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Probing the Physical Conditions of Atomic Gas at High Redshift

, , and . (2014)cite arxiv:1411.5027Comment: 21 Pages, 11 figures, comments welcome.

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Metallicity Evolution of Damped Lyman-alpha Systems out to z~5, , , , and . (2012)cite arxiv:1205.5047Comment: Accepted for publication in the Astrophysical Journal. 24 pages, 17 figures.The Fundamental Plane of Damped Lyman Alpha Systems, , , and . (2013)cite arxiv:1303.7239Comment: 18 pages with 10 figures, Submitted to ApJ.CII 158 micron Emission from the Host Galaxies of Damped Lyman Alpha Systems, , , , , and . (2017)cite arxiv:1703.07797Comment: Science; 25 pages, 6 color figures; see https://vimeo.com/209248385 for a related movie.Probing the Physical Conditions of Atomic Gas at High Redshift, , and . (2014)cite arxiv:1411.5027Comment: 21 Pages, 11 figures, comments welcome.UVUDF: Ultraviolet Imaging of the Hubble Ultradeep Field with Wide-field Camera 3, , , , , , , , , and 16 other author(s). (2013)cite arxiv:1305.1357Comment: Submitted AJ.Spatially Resolved Emission of a High Redshift DLA Galaxy with the Keck/OSIRIS IFU, and . (2013)cite arxiv:1311.0045Comment: Submitted to ApJ.The Rapid Decline in Metallicity of Damped Ly-$\alpha$ Systems at $z\sim5$, , , , and . (2013)cite arxiv:1310.6042Comment: 6 pages, 4 figures, submitted to ApJL.C II radiative cooling of the Galactic diffuse interstellar medium: Insight about the star formation in Damped Lyman-alpha systems, , , , , and . (2016)cite arxiv:1606.04966Comment: 16 pages, 3 tables, 9 figures. Accepted for publication in ApJ. The definitive version will be available at http://iopscience.iop.org/0004-637X.