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KMOS-3D Reveals Low-Level Star Formation Activity in Massive Quiescent Galaxies at 0.7 < z < 2.7, , , , , , , , , and 16 other author(s). (2017)cite arxiv:1703.07778Comment: 7 pages, 5 figures, submitted to ApJ Letters.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.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.Spectroscopic Confirmation of an Ultra Massive and Compact Galaxy at z=3.35: A Detailed Look at an Early Progenitor of Local Most Massive Ellipticals, , , , , , , , , and . (2014)cite arxiv:1406.0002Comment: 15 pages, 7 figures. Submitted to ApJ. Comments welcome.X-shooter Spectroscopy and HST Imaging of 15 Ultra Massive Quiescent Galaxies at $z\gtrsim2$, , , , , , , , , and 16 other author(s). (2019)cite arxiv:1912.01619Comment: 30 pages, 10 figures, accepted in ApJ.The Grism Lens-Amplified Survey from Space (GLASS). V. Extent and spatial distribution of star formation in z~0.5 cluster galaxies, , , , , , , , , and 7 other author(s). (2015)cite arxiv:1511.00686Comment: 18 pages, 15 figures, accepted for publication in ApJ.The evolution of metallicity and metallicity gradients from z=2.7-0.6 with KMOS3D, , , , , , , , , and 21 other author(s). (2016)cite arxiv:1603.01139Comment: submitted to ApJ.Spatially-resolved dust maps from Balmer decrements in galaxies at z~1.4, , , , , , , , and . (2015)cite arxiv:1511.04443Comment: Submitted to ApJ Letters. Fig. 2. shows measured radial Balmer decrement profiles. Fig. 3 shows inferred dust gradients. Fig. 4 shows dust-corrected radial profiles of star formation and the likely growth of bulges in high mass galaxies through in-situ star formation.Where stars form: inside-out growth and coherent star formation from HST Halpha maps of 2676 galaxies across the main sequence at z~1, , , , , , , , , and 10 other author(s). (2015)cite arxiv:1507.03999Comment: Submitted to ApJ. Main results: Fig. 6 shows the scale lengths of ionized gas vs. stellar disks. Fig. 9 shows where Halpha in galaxies is enhanced above and suppressed below the star-forming main sequence. Data points for Halpha profiles are available upon request.First results from the VIRIAL survey: the stellar content of $UVJ$-selected quiescent galaxies at $1.5 < z < 2$ from KMOS, , , , , , , , , and 7 other author(s). (2015)cite arxiv:1503.08831Comment: 6 pages, 5 figures, accepted for publication in ApJL.