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Characterization of JWST science performance from commissioning

, , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , and . (2022)cite arxiv:2207.05632Comment: 60 pages, 30 figures.

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The Security of NTP's Datagram Protocol., , , , , and . Financial Cryptography, volume 10322 of Lecture Notes in Computer Science, page 405-423. Springer, (2017)Characterization of JWST science performance from commissioning, , , , , , , , , and 601 other author(s). (2022)cite arxiv:2207.05632Comment: 60 pages, 30 figures.CEERS Key Paper III: The Resolved Host Properties of AGN at 3 < z < 5 with JWST, , , , , , , , , and 49 other author(s). (2022)cite arxiv:2208.14480Comment: Submitted to ApJ; 12 Pages, 6 Figures.CEERS Key Paper I: An Early Look into the First 500 Myr of Galaxy Formation with JWST, , , , , , , , , and 57 other author(s). (2022)cite arxiv:2211.05792Comment: 41 pages, 20 figures, 6 tables, submitted to ApJL. Key results in Figures 13-15, discussed in Sections 7 and 8.First results from Faint Infrared Grism Survey (FIGS): first simultaneous detection of Lyman-\alpha emission and Lyman break from a galaxy at z=7.51, , , , , , , , , and 15 other author(s). (2016)cite arxiv:1605.06519Comment: Resubmitted after incorporating referee's comments.The rise and fall of the star formation histories of blue galaxies at redshifts 0.2<z<1.4, , , , and . (2012)cite arxiv:1210.0543Comment: 5 pages, 2 figures, 1 table. Submitted to ApJ Letters on 29th September 2012.Far-Ultraviolet Number Counts of Field Galaxies, , , , and . (2011)cite arxiv:1105.1398 Comment: Accepted for publication in ApJ, including 34 pages, 6 figures, and 2 tables.The Bursty Star Formation Histories of Low-mass Galaxies at $0.4<z<1$ Revealed by Star Formation Rates Measured from FUV and H$\beta$, , , , , , , , , and 10 other author(s). (2016)cite arxiv:1604.05314Comment: 10 pages, 7 figures. Submitted to ApJ. Comments welcome.Physical Properties of Sub-galactic Clumps at 0.5 $z łeq$ 1.5 in the UVUDF, , , , , , , , , and 1 other author(s). (2017)cite arxiv:1702.03038Comment: Accepted for publication in ApJ. 18 pages, 18 figures.Semi-analytic forecasts for JWST -- V. AGN luminosity functions and helium reionization at z = 2-7, , , , , , , and . (2021)cite arxiv:2109.13241Comment: 28 pages, 23 figures, accepted for publication in MNRAS.