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Galaxy Structure as a Driver of the Star Formation Sequence Slope and Scatter

, , , , , , , , , , , , , , and . (2015)cite arxiv:1508.04771Comment: Accepted for publication in the Astrophysical Journal Letters.

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Quiescent Galaxies in the 3D-HST Survey: Spectroscopic Confirmation of a Large Number of Galaxies with Relatively Old Stellar Populations at z~2, , , , , , , , , and 3 other author(s). (2013)cite arxiv:1305.1943Comment: 6 pages, 4 figures, resubmitted to the Astrophysical Journal Letters after minor revisions.The Milky Way has no thick disk, , and . (2011)cite arxiv:1111.6585.The High-Mass Stellar Initial Mass Function in M31 Clusters, , , , , , , , , and 9 other author(s). (2015)cite arxiv:1502.06621Comment: 11 pages, 7 Figures, submitted to ApJ. Comments welcome.A Three-Dimensional Map of Milky-Way Dust, , , , , , , , , and 6 other author(s). (2015)cite arxiv:1507.01005Comment: Accepted for publication in ApJ.The Payne: self-consistent ab initio fitting of stellar spectra, , , and . (2018)cite arxiv:1804.01530Comment: 21 pages, 17 figures, 1 table, submitted to ApJ.The z=7.54 Quasar ULAS J1342+0928 Is Hosted by a Galaxy Merger, , , , , , , , , and 2 other author(s). (2019)cite arxiv:1909.00027.The Pan-STARRS1 $z>5.6$ Quasar Survey: III. The $z\approx6$ Quasar Luminosity Function, , , , , , , , , and 2 other author(s). (2022)cite arxiv:2212.04179Comment: ApJ accepted, 40 pages, 19 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.Characterization of JWST science performance from commissioning, , , , , , , , , and 601 other author(s). (2022)cite arxiv:2207.05632Comment: 60 pages, 30 figures.Spectroscopic Redshifts for Seven Lens Galaxies, , , , and . (October 2005)