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Where stars form: inside-out growth and coherent star formation from HST Halpha maps of 2676 galaxies across the main sequence at z~1, , , , , , , , , and 10 other author(s). (2015)cite arxiv:1507.03999Comment: Submitted to ApJ. Main results: Fig. 6 shows the scale lengths of ionized gas vs. stellar disks. Fig. 9 shows where Halpha in galaxies is enhanced above and suppressed below the star-forming main sequence. Data points for Halpha profiles are available upon request.Confirmation of Small Dynamical and Stellar Masses for Extreme Emission Line Galaxies at z~2, , , , , , , , , and 14 other author(s). (2013)cite arxiv:1310.6358Comment: Accepted for publication in ApJL, 5 pages, 1 table, 4 figures.A highly magnified candidate for a young galaxy seen when the Universe was 500 Myrs old, , , , , , , , , and 26 other author(s). (2012)cite arxiv:1204.2305Comment: Submitted to the Nature Journal. 39 Pages, 13 figures.CANDELS: Constraining the AGN-Merger Connection with Host Morphologies at z~2, , , , , , , , , and 28 other author(s). (2011)cite arxiv:1109.2588 Comment: 10 Pages, 5 Figures, Revised draft submitted to ApJ.CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey, , , , , , , , , and 96 other author(s). (2011)cite arxiv:1105.3753.CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey - The Hubble Space Telescope Observations, Imaging Data Products and Mosaics, , , , , , , , , and 112 other author(s). (2011)cite arxiv:1105.3754 Comment: 36 pages, 22 figures.Smooth(er) Stellar Mass Maps in CANDELS: Constraints on the Longevity of Clumps in High-redshift Star-forming Galaxies, , , , , , , , , and 15 other author(s). (2012)cite arxiv:1203.2611Comment: Submitted to The Astrophysical Journal, 25 pages, 1 table, 14 figures.Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?, , , , , , , , , and 15 other author(s). (2022)cite arxiv:2208.02794Comment: Submitted to ApJL. Fig. 1 shows the "superposed" state, Fig. 2 presents the potential z~5 protocluster, Fig. 3 shows some atypical z~5 SEDs, Fig. 4 studies the morphology, Fig. 5 summarizes the extraordinary situation at z~17, and Fig. 6 argues for why such interlopers may not be a major issue for z>10 searches. Comments warmly welcomed.The colors and sizes of recently quenched galaxies: a result of compact starburst before quenching, , , , , , , , , and 4 other author(s). (2019)cite arxiv:1912.03683Comment: 16 pages, 8 figures, 1 table, accepted by ApJ.CLASH: Three Strongly Lensed Images of a Candidate z ~ 11 Galaxy, , , , , , , , , and 13 other author(s). (2012)cite arxiv:1211.3663Comment: Accepted for publication in the Astrophysical Journal. 23 pages, 18 figures.