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The SINS/zC-SINF Survey of $z\sim2$ Galaxy Kinematics: Rest-frame Morphology, Structure, and Colors from Near-infrared Hubble Space Telescope Imaging, , , , , , , , , and 7 other author(s). (2014)cite arxiv:1411.7034Comment: 25 pages (+11 pages appendix), 20 figures; re-submitted to ApJ after responding to the first referee report.The lesser role of starbursts for star formation at z=2, , , , , , , , , and 24 other author(s). (2011)cite arxiv:1108.0933Comment: Accepted for publication in ApJ Letters.Dust temperature and CO-to-H2 conversion factor variations in the SFR-M* plane, , , , , , , , , and 8 other author(s). (2012)cite arxiv:1210.2760Comment: Accepted for publication in Astronomy and Astrophysics (A&A); 15 pages, 6 figures.Building the cosmic infrared background brick by brick with Herschel/PEP, , , , , , , , , and 17 other author(s). (2011)cite arxiv:1106.3070Comment: Proposed for acceptance on A&A.The SINS/zC-SINF survey of z~2 galaxy kinematics: Evidence for powerful AGN-driven nuclear outflows in massive star-forming galaxies, , , , , , , , , and 22 other author(s). (2013)cite arxiv:1311.2596Comment: 17 pages, 5 figures, submitted to Astrophysical Journal.Reversal or no reversal: the evolution of the star formation rate-density relation up to z~1.6?, , , , , , , , , and 20 other author(s). (2013)cite arxiv:1310.1398Comment: Accepted for publication in MNRAS.The SINS/zC-SINF survey of z~2 galaxy kinematics: evidence for gravitational quenching, , , , , , , , , and 18 other author(s). (2013)cite arxiv:1310.3838Comment: submitted to ApJ.PHIBSS: molecular gas content and scaling relations in z~1-3 normal star forming galaxies, , , , , , , , , and 14 other author(s). (2012)cite arxiv:1211.5743Comment: Submitted to the Astrophysical Journal; 14 figures.Non-linearity and environmental dependence of the star forming galaxies Main Sequence, , , , , , , , , and 23 other author(s). (2015)cite arxiv:1511.01899Comment: 14 pages, 14 figures, accepted for publication in MNRAS.KMOS^3D: Dynamical constraints on the mass budget in early star-forming disks, , , , , , , , , and 19 other author(s). (2016)cite arxiv:1603.03432Comment: Submitted to ApJ. Fig. 4 compares stellar and baryonic masses to dynamical masses. Fig. 6 and 7 show the dependence of stellar and baryonic mass fractions on redshift and surface density.