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The Faint-end of the UV Luminosity Function at z~6 to z~8: Combined Constraints from the Hubble Frontier Fields Clusters and Parallels, , , , , , , , , и 1 other автор(ы). (2015)cite arxiv:1509.06764Comment: 13 pages, 10 figures, 4 tables, submitted to ApJ.A bright lensed galaxy at $z=5.4$ with strong Ly$\alpha$ emission, , , , , , , , , и 3 other автор(ы). (2017)cite arxiv:1706.09428Comment: 19 pages, 13 figures, submitted to MNRAS.Early Science with the Large Millimeter Telescope: Detection of dust emission in multiple images of a normal galaxy at $z>4$ lensed by a Frontier Fields cluster, , , , , , , , , и 25 other автор(ы). (2017)cite arxiv:1703.04535Comment: 12 pages, 6 figures, accepted for publication in ApJ.The Evolution Of The Faint End Of The UV Luminosity Function During The Peak Epoch Of Star Formation (1<z<3), , , , , , , , , и 2 other автор(ы). (2016)cite arxiv:1606.00469Comment: 22 pages, 15 figures.Cosmological Constraints from Strong Gravitational Lensing in Clusters of Galaxies, , , , , , и . Science, 329 (5994): 924-927 (2010)High-redshift supernova rates measured with the gravitational telescope A1689, , , , , , , , , и 5 other автор(ы). (2016)cite arxiv:1607.01617Comment: Manuscript accepted for publication in Section 4. Extragalactic astronomy of Astronomy and Astrophysics. 22 pages, 13 figures.