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CO excitation of normal star forming galaxies out to $z=1.5$ as regulated by the properties of their interstellar medium

, , , , , , , , , , , , , , , , , and . (2014)cite arxiv:1409.8158Comment: 18 pages, 17 figures, 4 tables, submitted to A&A.

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A Molecular Line Scan in the Hubble Deep Field North: Constraints on the CO Luminosity Function and the Cosmic H2 Density, , , , , , , , , and 12 other author(s). (2013)cite arxiv:1312.6365Comment: Accepted for publication in ApJ.Dust and Gas in Star Forming Galaxies at z~3 - Extending Galaxy Uniformity to 11.5 Billion Years, , , , , , , , , and 3 other author(s). (2017)cite arxiv:1705.06296Comment: Accepted for publication at A&A.Dissecting the stellar mass-SFR correlation in z=1 star-forming disk galaxies, , , , , , , and . (2012)cite arxiv:1206.1704Comment: 6 pages, 4 figures, 1 table. ApJ Letters in press.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.ALMA and Herschel reveal that AGN and main-sequence galaxies have different star formation rate distributions, , , , , , , , , and 8 other author(s). (2015)cite arxiv:1506.05459Comment: 5 pages, 3 figures, 1 table; Submitted to MNRAS.GOODS-Herschel~: Gas-to-dust mass ratios and CO-to-H_2 conversion factors in normal and starbursting galaxies at high-z, , , , , , , , , and 8 other author(s). (2011)cite arxiv:1109.1140 Comment: Accepted for publication in ApJ.The VLA-COSMOS 3 GHz Large Project: The cosmic star formation history since z~5, , , , , , , , , and 12 other author(s). (2017)cite arxiv:1703.09724Comment: 18 pages, 8 figures.The Evolving Interstellar Medium of Star Forming Galaxies Since z=2 as Probed by Their Infrared Spectral Energy Distributions, , , , , , , , , and 4 other author(s). (2012)cite arxiv:1210.1035Comment: To appear in ApJ, in the November 10, 2012, v759 -2 issue.The implications of the surprising existence of a large, massive CO disk in a distant protocluster, , , , , , , , , and 11 other author(s). (2017)cite arxiv:1701.05250Comment: Submitted to A&A. 14 pages, 8 figures and 4 tables. Comments are welcomed.Semiconductor laser physics, , and . Springer, Berlin, (1994)