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COSMOS2020: A panchromatic view of the Universe to $z\sim10$ from two complementary catalogs, , , , , , , , , и 47 other автор(ы). (2021)cite arxiv:2110.13923Comment: 39 pages, 21 figures, accepted for publication in The Astrophysical Journal Supplement Series. Production of IRAC mosaics are presented in Moneti et al. "Euclid Preparation: XVIII. Cosmic Dawn Survey. Spitzer observations of the Euclid deep fields and calibration fields" which has been posted simultaneously. Catalogs can be accessed online now at https://cosmos2020.calet.org.The ALPINE-ALMA CII Survey: nature, luminosity function and star formation history of continuum non-target galaxies up to z~6, , , , , , , , , и 23 other автор(ы). (2020)cite arxiv:2006.04974Comment: 23 pages, 14 figures. Submitted to A&A. This paper is related to the two other ALPINE papers submitted today by Loiacono and Yan.The VLA-COSMOS 3 GHz Large Project: The cosmic star formation history since z~5, , , , , , , , , и 12 other автор(ы). (2017)cite arxiv:1703.09724Comment: 18 pages, 8 figures.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.Spitzer bright, UltraVISTA faint sources in COSMOS: the contribution to the overall population of massive galaxies at z=3-7, , , , , , , , , и . (2015)cite arxiv:1505.05721Comment: 16 pages, 13 figures, 4 tables. Submitted to the ApJ.The VIMOS Ultra-Deep Survey: ~10,000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2<z<~6, , , , , , , , , и 35 other автор(ы). (2014)cite arxiv:1403.3938Comment: 43 pages, 30 figures, submitted to A&A.The evolution of the star formation activity per halo mass up to redshift ~ 1.6 as seen by Herschel, , , , , , , , , и 33 other автор(ы). (2011)cite arxiv:1110.2946 Comment: 8 pages, 3 figures, accepted for publication on A&amp;A.A Dark Core in Abell 520, , , , и . (2007)Dust-obscured star formation and the contribution of galaxies escaping UV/optical color selections at z~2, , , , , , , , , и . (2011)cite arxiv:1106.0498Comment: Accepted for publication in A&amp;A. 16 pages, 13 figures.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.