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CO, H2O, H2O+ line and dust emission in a z = 3.63 strongly lensed starburst merger at sub-kiloparsec scales, , , , , , , , , and 15 other author(s). (2019)cite arxiv:1903.00273Comment: A&A accepted, 23 pages.Physical conditions of the interstellar medium of high-redshift, strongly lensed submillimetre galaxies from the Herschel-ATLAS, , , , , , , , , and 43 other author(s). (2011)cite arxiv:1105.3924 Comment: 13 pages, 6 figures, accepted in MNRAS.ALMA spectroscopic survey in the Hubble Ultra Deep Field: CO luminosity functions and the evolution of the cosmic density of molecular gas, , , , , , , , , and 30 other author(s). (2016)cite arxiv:1607.06770Comment: Submitted to the Astrophysical Journal, incorporating the first round of referee comments.Evolution of Interstellar Medium, Star Formation, and Accretion at High Redshift, , , , , , , , , and 13 other author(s). (2017)cite arxiv:1702.04729.The suppression of star formation by powerful active galactic nuclei, , , , , , , , , and 68 other author(s). (2013)cite arxiv:1310.4147Comment: Published in Nature, May 2012. Includes supplementary information.The SCUBA-2 Cosmology Legacy Survey: the submillimetre properties of Lyman break galaxies at z=3-5, , , , , , , , , and 21 other author(s). (2014)cite arxiv:1407.6712Comment: 12 pages, 8 figures, submitted to MNRAS.ALMACAL II: Extreme star-formation-rate densities in a pair of dusty starbursts at $z = 3.442$ revealed by ALMA 20-milliarcsec resolution imaging, , , , and . (2016)cite arxiv:1607.06464Comment: Submitted to ApJ. Comments are welcome.ISM masses and the star formation law at Z = 1 to 6 // ALMA observations of dust continuum in 145 galaxies in the COSMOS survey field, , , , , , , , , and 10 other author(s). (2015)cite arxiv:1511.05149.ALMA reveals Strong CII emission in a galaxy embedded in a giant Lyman-alpha blob at z=3.1, , , , , , , , , and 14 other author(s). (2016)cite arxiv:1701.00043Comment: 6 pages, 4 figures, 1 table, accepted for publication in the Astrophysical Journal Letters.An imperfectly passive nature: Bright sub-millimeter emission from dust-obscured star formation in the z=3.717 "passive" system, ZF20115, , , , , , , , , and 21 other author(s). (2017)cite arxiv:1704.03868Comment: ApJ submitted. Comments welcome.