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Evaluation of Climate Models., , , , , , , , , and 7 other author(s). Climate Change 2013: The Physical Science Basis. Contribution of Working Group I to the Fifth Assessment Report of the Intergovernmental Panel on Climate Change, Cambridge University Press, Cambridge, United Kingdom and New York, NY, USA., (2013)An Overview of the 2014 ALMA Long Baseline Campaign, , , , , , , , , and 240 other author(s). (2015)cite arxiv:1504.04877Comment: 11 pages, 7 figures, 2 tables; accepted for publication in the Astrophysical Journal Letters.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.CO emission in optically obscured (type-2) quasars at redshifts z=0.1-0.4, , and . (2012)cite arxiv:1205.1962Comment: accepted for publication in ApJ; 10 pages, 6 figures, 4 tables; format is emulateapj.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 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.An ALMA survey of sub-millimeter galaxies in the Extended Chandra Deep Field South: Sub-millimeter properties of color-selected galaxies, , , , , , , , , and 9 other author(s). (2013)cite arxiv:1311.2604Comment: 9 figures. Accepted for publication in ApJ.An improved representation of physical permafrost dynamics in the JULES land surface model, , , , , , , and . Geoscientific Model Development Discussions, 8 (1): 715--759 (Jan 30, 2015)Moses 2.2 Technical Documentation, , and . 30. Hadley Centre, (2001)Molecular Gas in Infrared Ultraluminous QSO Hosts, , , , , , , , and . (2012)cite arxiv:1202.6490Comment: 30 pages, 9 figures, accepted for publication in The Astrophysical Journal.