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Evidence for Wide-Spread AGN Driven Outflows in the Most Massive z~1-2 Star Forming Galaxies, , , , , , , , , and 28 other author(s). (2014)cite arxiv:1406.0183Comment: 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.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.The KMOS^3D Survey: design, first results, and the evolution of galaxy kinematics from 0.7<z<2.7, , , , , , , , , and 17 other author(s). (2014)cite arxiv:1409.6791Comment: 20 pages, 11 figures, submitted to ApJ.The angular momentum distribution and baryon content of star forming galaxies at z~1-3, , , , , , , , , and 18 other author(s). (2015)cite arxiv:1510.03262Comment: Submitted to Astrophysical Journal.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.The Nature of Star Formation at 24 microns in the Group Environment at 0.3 &lt; z &lt; 0.55, , , , , , , , , and . (2011)cite arxiv:1107.2431Comment: Accepted to ApJ. 44 pages, 13 figures.