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Do galaxies that leak ionizing photons have extreme outflows?, , , , , , , и . (2017)cite arxiv:1707.01913Comment: 17 pages, 8 Figures. Accepted for publication in Astronomy & Astrophysics.Detection of high Lyman continuum leakage from four low-redshift compact star-forming galaxies, , , , , и . (2016)cite arxiv:1605.05160Comment: 21 pages, 14 figures, accepted for publication in MNRAS.The ionizing photon production efficiency of compact z~0.3 Lyman continuum leakers and comparison with high redshift galaxies, , , , , , и . (2016)cite arxiv:1606.00053Comment: Accepted for publication in A&A Letters.ALMA reveals metals yet no dust within multiple components in CR7, , , , , , , , , и 1 other автор(ы). (2017)cite arxiv:1709.06569Comment: 17 pages, submitted to ApJ, comments welcome.Molecular gas content in strongly-lensed z~1.5-3 star-forming galaxies with low IR luminosities, , , , , , , , , и 3 other автор(ы). (2014)cite arxiv:1408.0816Comment: 21 pages, 16 figures. Submitted to A&A.New constraints on dust emission and UV attenuation of z=6.5-7.5 galaxies from IRAM and ALMA observations, , , , , , , и . (2014)cite arxiv:1407.5793Comment: 10 pages, 8 figures. Submitted to A&A.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.No strong dependence of Lyman continuum leakage on physical properties of star-forming galaxies at $3.1 z 3.5$, , , , , , , , , и 8 other автор(ы). (2021)cite arxiv:2109.03662Comment: 18 pages, 11 figures, 1 appendix, submitted to Monthly Notices of the Royal Astronomical Society.The VIMOS Ultra Deep Survey: Emerging from the Dark, a Massive Proto-Cluster at z~4.57, , , , , , , , , и 13 other автор(ы). (2017)cite arxiv:1703.10170Comment: 26 pages, 14 figures, 1 table, submitted to A&A.The VIMOS Ultra-Deep Survey: the Ly$\alpha$ emission line morphology at $2 < z < 6$, , , , , , , , , и 13 other автор(ы). (2020)cite arxiv:2007.01322Comment: 18 pages, 13 figures, submitted to A&A.