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The Mass Dependence of Star Formation Histories in Barred Spiral Galaxies

, , , and . (2016)cite arxiv:1610.02366Comment: 15 pages, 14 figures.

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The chemistry of the most metal-rich damped Lyman $\alpha$ systems at z$\sim2$ II. Context with the Local Group, , , , and . (2015)cite arxiv:1507.08311Comment: Accepted for publication in MNRAS. 24 Pages, 10 Figures, 4 tables. Data compilations within tarball or available upon request (contact Trystyn Berg).Galaxy Pairs in the Sloan Digital Sky Survey - V. Tracing changes in star formation rate and metallicity out to separations of 80 kpc, , , , and . (2012)cite arxiv:1207.4791Comment: Accepted for publication in MNRAS. 18 pages, 13 figures.Variations in the slope of the resolved star-forming main sequence: a tool for constraining the mass of star-forming regions, , , , , , , and . (2019)cite arxiv:1912.04290Comment: submitted to MNRAS-Letters.Towards a physical picture of star-formation quenching: the photometric properties of recently-quenched galaxies in the Sloan Digital Sky Survey, , , and . (2012)cite arxiv:1211.6115Comment: 16 pages, 11 figures. Accepted for publication in MNRAS.Quasars Probing Quasars VI. Excess HI Absorption Within One Proper Mpc of z~2 Quasars, , , , , , , , , and 2 other author(s). (2013)cite arxiv:1308.6222Comment: Accepted to ApJ; 38 pages, 25 figures. Comments still welcome.The Mass Dependence of Star Formation Histories in Barred Spiral Galaxies, , , and . (2016)cite arxiv:1610.02366Comment: 15 pages, 14 figures.Galaxy pairs in the Sloan Digital Sky Survey - VI. The orbital extent of enhanced star formation in interacting galaxies, , , , and . (2013)cite arxiv:1305.1595Comment: 6 pages, 4 figures. Accepted for publication in MNRAS Letters.From Exoplanets to Quasars: Detection of Potential Damped Lyman Alpha Absorbing Galaxies Using Angular Differential Imaging, , and . (2016)cite arxiv:1609.00384.Sub-damped Lyman alpha systems in the XQ-100 survey II -- Chemical evolution at 2.4<z<4.3, , , , , , , , , and 1 other author(s). (2021)cite arxiv:2101.07821Comment: Accepted for publication in MNRAS. 64 pages (20 pages of main text, 44 pages of Figures in appendix). Machine-readable versions of Tables 2 and 3 are available in the source files or available online on MNRAS.The Neutral Hydrogen Cosmological Mass Density at z=5, , , , , , , , , and 1 other author(s). (2015)cite arxiv:1506.02037Comment: Accepted by MNRAS. Comments and reference suggestions are still welcome. Data and code for the paper will appear at https://github.com/nhmc/GGG_DLA after the final version has been published.