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A higher efficiency of converting gas to stars push galaxies at z ~ 1.6 well above the star-forming main sequence, , , , , , , , , and 10 other author(s). (2015)cite arxiv:1505.04977Comment: Submitted to ApJ Letters; 6 pages, 4 figures.Massive Molecular Outflows and Evidence for AGN Feedback from CO Observations, , , , , , , , , and 5 other author(s). (2013)cite arxiv:1311.2595Comment: 26 pages, Accepted for publication in A&A, abstract abridged due to arXiv requirements.A direct constraint on the gas content of a massive, passively evolving elliptical galaxy at z = 1.43, , , , , , , , and . (2015)cite arxiv:1502.00003Comment: 6 pages, 3 figures & 1 table. Submitted to ApJL.Mapping metals at high redshift with far-infrared lines, , , , , , and . (2015)cite arxiv:1506.05803Comment: 12 pages, 6 figures; submitted to MNRAS.The Discovery of Gas-Rich, Dusty Starbursts in Luminous Reddened Quasars at $z\sim2.5$ with ALMA, , , , , , , and . (2016)cite arxiv:1610.04907Comment: Re-submitted to MNRAS following referee's report.The Molecular Gas Content of z = 3 Lyman Break Galaxies; Evidence of a non Evolving Gas Fraction in Main Sequence Galaxies at z > 2, , , , , , , , , and 3 other author(s). (2012)cite arxiv:1209.1484Comment: Accepted for publication in ApJL.Evidence for feedback in action from the molecular gas content in the z~1.6 outflowing QSO XID2028, , , , , , , , , and 9 other author(s). (2015)cite arxiv:1503.01783Comment: 8 pages, 4 figures. Astronomy and Astrophysics, in press.Ionised outflows in z $\sim$ 2.4 quasar host galaxies, , , , , , , , , and 10 other author(s). (2015)cite arxiv:1506.03096Comment: 13 pages, 11 figures; accepted for publication in A&A.The MAGNUM survey: Positive feedback in the nuclear region of NGC 5643 suggested by MUSE, , , , , , , , , and 11 other author(s). (2015)cite arxiv:1508.04464Comment: 9 pages, 7 figures, accepted for publication in A&A.A Molecular gas rich GRB host galaxy at the peak of cosmic star formation with significant outflowing gas, , , , , , , , , and 3 other author(s). (2017)cite arxiv:1709.00424Comment: Submitted to MNRAS Letters.