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The Physical Conditions, Metallicity and Metal Abundance Ratios In a Highly Magnified Galaxy at z = 3.6252, , , , , , , и . (2013)cite arxiv:1310.6695Comment: emulate ApJ format, 19 pages, 9 figures, 7 tables. Submitted to ApJ. Comments welcome.Spatially Resolved Patchy Lyman-$\alpha$ Emission Within the Central Kiloparsec of a Strongly Lensed Quasar Host Galaxy at z = 2.8, , , , , , , , , и 3 other автор(ы). (2017)cite arxiv:1708.00453Comment: Accepted to ApJ Letters; 7 pages, 5 figures.HST-Based Lens Model of the First Extragalactic JWST Science Target, SDSS J1226+2152, in Preparation for TEMPLATES, , , , , , , и . (2022)cite arxiv:2207.05709Comment: 13 pages, 7 figures. Submitted to ApJ. Data to be posted soon at MAST at http://dx.doi.org/10.17909/zqax-2y86.A Thirty Kiloparsec Chain of "Beads on a String" Star Formation Between Two Merging Early Type Galaxies in the Core of a Strong-Lensing Galaxy Cluster, , , , , , , , , и 3 other автор(ы). (2014)cite arxiv:1407.2251Comment: 7 pages, 4 figures, accepted for publication in ApJ Letters. High resolution images of the cluster can be found at http://hubblesite.org/news/2014/26.Constraints on the low-mass end of the mass-metallicity relation at z=1-2 from lensed galaxies, , , и . (2012)cite arxiv:1202.5267Comment: 16 pages, 9 figures, submitted to the Astrophysical Journal.Resolved Star Formation on Sub-galactic Scales in a Merger at z=1.7, , , , , , и . (2014)cite arxiv:1405.0490Comment: 14 pages, 8 figures. Re-submitted to ApJ.How dark the sky: the JWST backgrounds, , , , , , , , , и 10 other автор(ы). (2022)cite arxiv:2211.09890Comment: Submitted to the "JWST Overview" special issue of PASP.Galaxy Structure as a Driver of the Star Formation Sequence Slope and Scatter, , , , , , , , , и 5 other автор(ы). (2015)cite arxiv:1508.04771Comment: Accepted for publication in the Astrophysical Journal Letters.C III Emission in Star-Forming Galaxies Near and Far, , , , , , , и . (2015)cite arxiv:1510.02542Comment: 4 figures, 1 table; Accepted for publication in ApJ Letters.