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Characterization of JWST science performance from commissioning, , , , , , , , , and 601 other author(s). (2022)cite arxiv:2207.05632Comment: 60 pages, 30 figures.ALMA 200 pc imaging of a z~7 quasar reveals a compact, disk-like host galaxy, , , , , , , , , and 3 other author(s). (2022)cite arxiv:2201.06396Comment: Accepted for publication in The Astrophysical Journal.Spectroscopic Redshifts for Seven Lens Galaxies, , , , and . (October 2005)Spatially resolved Halpha maps and sizes of 57 strongly star-forming galaxies at z~1 from 3D-HST: evidence for rapid inside-out assembly of disk galaxies, , , , , , , , , and 6 other author(s). (2012)cite arxiv:1202.1822 Comment: ApJ Letters, in press. The public 3D-HST website is http://3dhst.research.yale.edu/Home.html.Halpha Equivalent Widths from the 3D-HST survey: evolution with redshift and dependence on stellar mass, , , , , , , , , and 5 other author(s). (2012)cite arxiv:1206.2645Comment: Submitted to 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.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.ALMA spectroscopic survey in the Hubble Ultra Deep Field: CO luminosity functions and the evolution of the cosmic density of molecular gas, , , , , , , , , and 30 other author(s). (2016)cite arxiv:1607.06770Comment: Submitted to the Astrophysical Journal, incorporating the first round of referee comments.Observations of environmental quenching in groups in the 11 Gyr since z=2.5: different quenching for central and satellite galaxies, , , , , , , , , and 9 other author(s). (2014)cite arxiv:1401.2984Comment: Submitted to ApJ.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.