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Dust and Gas in Star Forming Galaxies at z~3 - Extending Galaxy Uniformity to 11.5 Billion Years

, , , , , , , , , , , , and . (2017)cite arxiv:1705.06296Comment: Accepted for publication at 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.High-resolution spectroscopic imaging of CO in a z=4.05 proto-cluster, , , , and . (2013)cite arxiv:1307.4763Comment: Accepted to ApJ.MOONS: a multi-object optical and near-infrared spectrograph for the VLT, , , , , , , , , and 70 other author(s). Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, volume 8446 of Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, (September 2012)The kiloparsec-scale star formation law at redshift 4: wide-spread, highly efficient star formation in the dust-obscured starburst galaxy GN20, , , , , , and . (2014)cite arxiv:1412.2132Comment: 6 pages, 5 figures, accepted to ApJL.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.Predicting emission line fluxes and number counts of distant galaxies for cosmological surveys, , , , , , , , , and 2 other author(s). (2017)cite arxiv:1709.01936Comment: Accepted for publication in MNRAS. 21 pages (+9 pages of appendix), 18 Figures. Machine readable tables will be available online.The evolution of the star formation activity per halo mass up to redshift ~ 1.6 as seen by Herschel, , , , , , , , , and 33 other author(s). (2011)cite arxiv:1110.2946 Comment: 8 pages, 3 figures, accepted for publication on A&A.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.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.