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The redshift evolution of rest-UV spectroscopic properties in Lyman Break Galaxies at z ~ 2-4

, , , , , , , , , , and . (2018)cite arxiv:1803.05912Comment: 27 pages, 14 figures, submitted to ApJ.

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The redshift evolution of rest-UV spectroscopic properties in Lyman Break Galaxies at z ~ 2-4, , , , , , , , , and 1 other author(s). (2018)cite arxiv:1803.05912Comment: 27 pages, 14 figures, submitted to ApJ.An Unsupervised Hunt for Gravitational Lenses., , , , and . AISTATS, volume 151 of Proceedings of Machine Learning Research, page 9827-9843. PMLR, (2022)Keck Spectroscopy of Gravitationally Lensed z=4 Galaxies: Improved Constraints on the Escape Fraction of Ionizing Photons, , , and . (2013)cite arxiv:1304.7015Comment: submitted to ApJ.Testing the Universality of the Fundamental Metallicity Relation at High Redshift Using Low-Mass Gravitationally Lensed Galaxies, , , and . (2013)cite arxiv:1302.3614Comment: Submitted to ApJ, 14 pages, 8 figures.The Origin and Evolution of Metallicity Gradients: Probing the Mode of Mass Assembly at z=2, , , and . (2012)cite arxiv:1207.4489Comment: Submitted to ApJ.Early Results from GLASS-JWST. I: Confirmation of Lensed $z\geqslant7$ Lyman-Break Galaxies Behind the Abell 2744 Cluster With NIRISS, , , , , , , , , and 22 other author(s). (2022)cite arxiv:2207.11387Comment: Submitted to ApJL. 10 pages, 3 figures, 1 table.A strong He II $łambda$1640 emitter with extremely blue UV spectral slope at $z=8.16$: presence of Pop III stars?, , , , , , , , , and 1 other author(s). (2022)cite arxiv:2212.04476Comment: Submitted.ALMA CII detection of a redshift 7 lensed galaxy behind RXJ1347.1-1145, , , , , , , , , and 6 other author(s). (2016)cite arxiv:1610.02099Comment: Submitted for publication to ApJLetters.Improving $z\sim7-11$ Galaxy Property Estimates with JWST/NIRCam Medium-Band Photometry, , , , , and . (2021)cite arxiv:2102.04469Comment: 13 pages, 7 figures. Accepted for publication in ApJ.A massive interacting galaxy 525 million years after the Big Bang, , , , , , , , , and 17 other author(s). (2023)cite arxiv:2303.00306Comment: 52 pages, 10 figures.