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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.Very High Gas Fractions and Extended Gas Reservoirs in z = 1.5 Disk Galaxies, , , , , , , , , and 3 other author(s). \apj, (April 2010)CO excitation of normal star forming galaxies out to $z=1.5$ as regulated by the properties of their interstellar medium, , , , , , , , , and 8 other author(s). (2014)cite arxiv:1409.8158Comment: 18 pages, 17 figures, 4 tables, submitted to A&A.Evolution of the mass, size, and star formation rate in high-redshift galaxies MIRAGE - A new sample of simulations with detailed stellar feedback, , , , , , , and . (2013)cite arxiv:1307.7130Comment: 18 pages, 12 figures.Metal deficiency in cluster star-forming galaxies at z=2, , , , , , , , , and 1 other author(s). (2014)cite arxiv:1410.1437Comment: 18 pages, 18 figures, Submitted to ApJ.A superluminous supernova in high surface density molecular gas within the bar of a metal-rich galaxy, , , , , , , , , and 1 other author(s). (2019)cite arxiv:1906.00972Comment: Accepted for publication in the Astrophysical Journal (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.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.The surprisingly large dust and gas content of quiescent galaxies at z>1.4, , , , , , , , , and 6 other author(s). (2017)cite arxiv:1703.02207Comment: 6 pages, 4 figures (main); 9 pages, 6 figures (supplementary); submitted to Nature Astronomy, comments welcome.Modelling CO emission from hydrodynamic simulations of nearby spirals, starbursting mergers, and high-redshift galaxies, , , , , and . (2014)cite arxiv:1409.8157Comment: submitted to A&A.