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When Spectral Modeling Meets Convolutional Networks: A Method for Discovering Reionization-era Lensed Quasars in Multi-band Imaging Data.

, , , , , , , , , , and . CoRR, (2022)

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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.The Number Density Evolution of Extreme Emission Line Galaxies in 3D-HST: Results from a Novel Automated Line Search Technique for Slitless Spectroscopy, , , , , , , , and . (2016)cite arxiv:1608.01674Comment: 14 pages, 11 Figures; Resubmitted to ApJ after addressing referee comments.The Assembly of Milky Way-like Galaxies Since z~2.5, , , , , , , , , and 9 other author(s). (2013)cite arxiv:1304.2391Comment: Submitted to ApJ Letters. 7 pages, 5 figures.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.Not In Our Backyard: Spectroscopic Support for the CLASH z=11 Candidate MACS0647-JD, , , , , , , , , and 5 other author(s). (2015)cite arxiv:1502.05681Comment: 14 Pages. 6 Figures. 2nd revised version. To appear in ApJ. Please contact npirzkal@stsci.edu for comments on this paper.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.Shape Evolution of Massive Early-Type Galaxies: Confirmation of Increased Disk Prevalence at z>1, , , , , , and . (2012)cite arxiv:1211.2113Comment: accepted for publication in ApJ; 11 pages; 10 figures; 4 tables.Galaxy Structure as a Driver of the Star Formation Sequence Slope and Scatter, , , , , , , , , and 5 other author(s). (2015)cite arxiv:1508.04771Comment: Accepted for publication in the Astrophysical Journal Letters.The Radial Distribution of Star Formation in Galaxies at z~1 from the 3D-HST Survey, , , , , , , , , and 9 other author(s). (2013)cite arxiv:1301.0320Comment: Accepted for publication in ApJ Letters.