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The Interstellar Medium In Galaxies Seen A Billion Years After The Big Bang

, , , , , , , , , , , , , and . (2015)cite arxiv:1503.07596Comment: Submitted to Nature, under review after referee report. 22 pages, 4 figures, 4 Extended Data Figures, 5 Extended Data tables.

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ISM Masses and Star Formation at z = 1 to 6 ALMA Observations of Dust Continuum in 180 Galaxies in COSMOS, , , , , , , , , and 5 other author(s). (2015)cite arxiv:1505.02159Comment: submitted ApJ Letters.The Interstellar Medium In Galaxies Seen A Billion Years After The Big Bang, , , , , , , , , and 4 other author(s). (2015)cite arxiv:1503.07596Comment: Submitted to Nature, under review after referee report. 22 pages, 4 figures, 4 Extended Data Figures, 5 Extended Data tables.The Calibration of Mid-Infrared Star Formation Rate Indicators, , , , , , , , , and 18 other author(s). \apj, (September 2007)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.Environmental Effect on the Interstellar Medium in Galaxies across the Cosmic Web at z=0.73, , , , , , and . (2019)cite arxiv:1902.08216Comment: Accepted for publication in ApJ.Evolution of Interstellar Medium, Star Formation, and Accretion at High Redshift, , , , , , , , , and 13 other author(s). (2017)cite arxiv:1702.04729.Evolution of the specific Star Formation Rate Function at z<1.4 - Dissecting the mass-SFR plane in COSMOS and GOODS, , , , , , , , , and 12 other author(s). (2014)cite arxiv:1410.4875Comment: 24 pages, 15 figures, 3 tables, submitted to A&A, comments are welcome.The Evolution of ISM Mass Probed by Dust Emission -- ALMA Observations at z = 0.3 to 2, , , , , , , , , and 2 other author(s). (2014)cite arxiv:1401.2987Comment: Accepted ApJ 1/13/2014.Development and Validation of a Thermal Model for Electric Induction Motors, , , , , , , and . IEEE Transactions on Industrial Electronics, 57 (12): 4043-4054 (December 2010)Large scale bias and the peak background split, and . (1999)cite arxiv:astro-ph/9901122Comment: 8 pages, 6 figures, submitted to MNRAS corrected y-label for fig.4 (newlabel = 1 + oldlabel).