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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 Low-Redshift Lyman Continuum Survey: Optically Thin and Thick Mg II Lines as Probes of Lyman Continuum Escape, , , , , , , , , and 7 other author(s). (2023)cite arxiv:2301.04087Comment: 12 pages, 5 figures, 2 tables, accepted to ApJ.The BOSS Emission-Line Lens Survey. III. : Strong Lensing of Ly$\alpha$ Emitters by Individual Galaxies, , , , , , , , , and 1 other author(s). (2016)cite arxiv:1604.01842Comment: 15 pages, 5 figures, submitted to the ApJ.SHARDS Frontier Fields: Physical properties of a low mass Lyman-alpha emitter at z=5.75, , , , , , , , , and 13 other author(s). (2017)cite arxiv:1710.00826Comment: 14 pages, 8 figures, 4 tables. Accepted for publication in ApJ.The BOSS Emission-Line Lens Survey V. Morphology and Substructure of Lensed Lyman-$\alpha$ Emitters at redshift $z\approx2.5$ in the BELLS GALLERY, , , , , , , , , and 2 other author(s). (2017)cite arxiv:1708.08854Comment: 12 pages, 5 figures.