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The Evolving Interstellar Medium of Star Forming Galaxies Since z=2 as Probed by Their Infrared Spectral Energy Distributions

, , , , , , , , , , , , , and . (2012)cite arxiv:1210.1035Comment: To appear in ApJ, in the November 10, 2012, v759 -2 issue.

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Dust properties of Lyman break galaxies at $z\sim3$, , , , , , , , , and 11 other author(s). (2015)cite arxiv:1512.04120Comment: Accepted to A&A, 17 Pages, 14 Figures, 2 Tables.A Dust-Obscured Massive Maximum-Starburst Galaxy at a Redshift of 6.34, , , , , , , , , and 54 other author(s). (2013)cite arxiv:1304.4256Comment: 35 pages, 19 figures, 5 tables, including Supplementary Information (version formatted by the authors). To appear in Nature. Under press embargo until 18:00 London time/13:00 US Eastern Time on 17 April 2013.The hidden AGN main sequence: Evidence for a universal SMBH accretion to star formation rate ratio since z~2 producing a M_BH-M* relation, , , , , , , , and . (2012)cite arxiv:1204.2824Comment: 6 Pages, 3 Figures, Submitted to ApJL.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.Galaxy growth in a massive halo in the first billion years of cosmic history, , , , , , , , , and 27 other author(s). (2017)cite arxiv:1712.03020Comment: Nature, published online on 06 December 2017.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.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.On the redshift evolution (0 < z < 4) of dust attenuation and of the total (UV+IR) star formation rate density, , , , , , , , , and 12 other author(s). (2013)cite arxiv:1304.7000Comment: Submitted to A&A.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.A simple halo model formalism for the cosmic infrared background and its correlation with the thermal Sunyaev Zel'dovich effect, , and . (2020)cite arxiv:2006.16329Comment: 20 pages (3 in appendix), 13 figures (4 in appendix), submitted to A&A.