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The Evolution of ISM Mass Probed by Dust Emission -- ALMA Observations at z = 0.3 to 2, , , , , , , , , и 2 other автор(ы). (2014)cite arxiv:1401.2987Comment: Accepted ApJ 1/13/2014.Early Science with the Large Millimeter Telescope: CO and C II Emission in the z=4.3 AzTEC J095942.9+022938 (COSMOS AzTEC-1), , , , , , , , , и 20 other автор(ы). (2015)cite arxiv:1508.05425Comment: 16 pages, 12 figures, accepted for publication in the Monthly Notices of the Royal Astronomical Society.The Sloan Digital Sky Survey: Technical Summary, , , , , , , , , и 135 other автор(ы). \aj, (сентября 2000)Evolution of Interstellar Medium, Star Formation, and Accretion at High Redshift, , , , , , , , , и 13 other автор(ы). (2017)cite arxiv:1702.04729.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, , , , , , , , , и 10 other автор(ы). (2015)cite arxiv:1511.05149.ISM Masses and Star Formation at z = 1 to 6 ALMA Observations of Dust Continuum in 180 Galaxies in COSMOS, , , , , , , , , и 5 other автор(ы). (2015)cite arxiv:1505.02159Comment: submitted ApJ Letters.Dust attenuation in 2<z<3 star-forming galaxies from deep ALMA observations of the Hubble Ultra Deep Field, , , , , , , , , и 5 other автор(ы). (2017)cite arxiv:1709.06102Comment: 17 pages, 7 figures, submitted to MNRAS.The Sloan Digital Sky Survey: Technical Summary, , , , , , , , , и 134 other автор(ы). The Astronomical Journal, (сентября 2000)A deep ALMA image of the Hubble Ultra Deep Field, , , , , , , , , и 26 other автор(ы). (2016)cite arxiv:1606.00227Comment: 25 pages, 14 figures, submitted to MNRAS.Noise suppression using local acceleration feedback control of an active absorber., , , и . J. Syst. Control. Eng., 229 (6): 495-505 (2015)