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Enriched halos at redshift $z=2$ with no star-formation: Implications for accretion and wind scenarios

, , , , , , , , , , , and . (2011)cite arxiv:1107.4618 Comment: accepted for publication in MNRAS.

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Fine-Structure FeII* Emission and Resonant MgII Emission in z = 1 Star-Forming Galaxies, , , , , and . (2013)cite arxiv:1302.6997Comment: 30 pages, 22 figures, submitted to ApJ.The Emission-Line Spectra of Major Mergers: Evidence for Shocked Outflows, , , and . (2012)cite arxiv:1205.0083Comment: Submitted to ApJ. 12 Pages, 7 Figures, 1 Table. This is a companion paper to "Gas Excitation in ULIRGS: Maps of Diagnostic Emission-Line Ratios in Space and Velocity" by Soto & Martin 2012.Physical properties of galactic winds using background quasars, , , , , , and . (2011)cite arxiv:1110.5877 Comment: 14 pages, 13 figures, submitted to MNRAS.Enriched halos at redshift $z=2$ with no star-formation: Implications for accretion and wind scenarios, , , , , , , , , and 2 other author(s). (2011)cite arxiv:1107.4618 Comment: accepted for publication in MNRAS.Possible Signatures of a Cold-Flow Disk from MUSE using a z=1 galaxy--quasar pair towards SDSSJ1422-0001, , , , , , , , , and 12 other author(s). (2016)cite arxiv:1601.07567Comment: 17 pages, 11 figures, accepted for publication in ApJ.