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A gas cloud on its way towards the super-massive black hole in the Galactic Centre, , , , , , , , , and 2 other author(s). (2011)cite arxiv:1112.3264Comment: in press at Nature.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.Herschel-PACS Observations of Far-IR CO Line Emission in NGC 1068: Highly Excited Molecular Gas in the Circumnuclear Disk, , , , , , , , , and 6 other author(s). (2012)cite arxiv:1202.5746Comment: 18 pages, 10 figures. Submitted to ApJ.The metallicity dependence of the CO \rightarrow H_2 conversion factor in z>1 star forming galaxies, , , , , , , , , and 13 other author(s). (2011)cite arxiv:1106.2098Comment: submitted to ApJ.The evolution of the star formation activity per halo mass up to redshift ~ 1.6 as seen by Herschel, , , , , , , , , and 33 other author(s). (2011)cite arxiv:1110.2946 Comment: 8 pages, 3 figures, accepted for publication on A&A.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.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.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.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.