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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.

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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.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.Galaxies with Background QSOs, I: A Search for Strong Galactic H-alpha Lines, , , , , , , , , and 5 other author(s). (2012)cite arxiv:1204.5786.Ubiquitous giant Lyman $\alpha$ nebulae around the brightest quasars at $z\sim3.5$ revealed with MUSE, , , , , , , , , and 10 other author(s). (2016)cite arxiv:1605.01422Comment: 19 pages, 8 figures, 3 Tables, submitted to ApJ.Dark Galaxy Candidates at Redshift ~3.5 Detected with MUSE, , , , , , , , , and 11 other author(s). (2017)cite arxiv:1709.03522Comment: 28 pages, 13 figures, 5 tables, submitted to ApJ.The extent of chemically enriched gas around star-forming dwarf galaxies, , , , and . (2017)cite arxiv:1710.06441Comment: Accepted to ApJL, 10 pages, 3 figures, 2 tables.MusE GAs FLOw and Wind (MEGAFLOW) I: First MUSE results on background quasars, , , , , , , , , and 6 other author(s). (2016)cite arxiv:1605.03412Comment: 20 pages, 16 figures, submitted to ApJ.