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The evolution of the dust and gas content in galaxies, , , , , , , , , and 29 other author(s). (2013)cite arxiv:1311.3670Comment: Accepted for publication in A&A.Enriched halos at redshift $z=2$ with no star-formation: Implications for accretion and wind scenarios, , , , , , , , , and 2 other author(s). (2011)cite arxiv:1107.4618 Comment: accepted for publication in MNRAS.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 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&amp;A.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.ALMA observations of feeding and feedback in nearby Seyfert galaxies: an AGN-driven outflow in NGC 1433, , , , , , , , , and 2 other author(s). (2013)cite arxiv:1309.7486Comment: 11 pages, 9 figures, Accepted in Astronomy and Astrophysics.Molecular and atomic gas along and across the main sequence of star-forming galaxies, , , , , , , , , and 3 other author(s). (2016)cite arxiv:1607.05289Comment: 9 pages, 6 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.High Resolution Imaging of PHIBSS z~2 Main Sequence Galaxies in CO J=1-0, , , , , , , , , and 7 other author(s). (2015)cite arxiv:1507.05652Comment: To appear in 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.