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The KMOS Deep Survey (KDS) I: dynamical measurements of typical star-forming galaxies at z $\simeq$ 3.5, , , , , , , , , and . (2017)cite arxiv:1704.06263Comment: main body 25 pages, 8 figures.A massive quiescent galaxy at redshift 4.658, , , , , , , , , and 3 other author(s). (2023)cite arxiv:2301.11413Comment: 24 pages, 4 figures, submitted to Nature.A Dust-Obscured Massive Maximum-Starburst Galaxy at a Redshift of 6.34, , , , , , , , , and 54 other author(s). (2013)cite arxiv:1304.4256Comment: 35 pages, 19 figures, 5 tables, including Supplementary Information (version formatted by the authors). To appear in Nature. Under press embargo until 18:00 London time/13:00 US Eastern Time on 17 April 2013.A mass threshold in the number density of passive galaxies at z$\sim$2, , , , , , , , , and 9 other author(s). (2014)cite arxiv:1409.7083Comment: Accepted for publication on Astronomy and Astrophysics.Chasing passive galaxies in the early Universe: a critical analysis in CANDELS GOODS-South, , , , , , , , , and 5 other author(s). (2017)cite arxiv:1709.00429Comment: 28 pages, 13 figures, 2 tables.The VANDELS survey: Dust attenuation in star-forming galaxies at $z=3-4$, , , , , , , , , and 7 other author(s). (2017)cite arxiv:1712.01292Comment: 15 pages, 11 figures, submitted to MNRAS.High velocity outflows from young star-forming galaxies in the UKIDSS Ultra-Deep Survey, , , , , , , , , and 3 other author(s). (2013)cite arxiv:1304.7276Comment: 16 pages, 15 figures, accepted by MNRAS.Dust attenuation in 2<z<3 star-forming galaxies from deep ALMA observations of the Hubble Ultra Deep Field, , , , , , , , , and 5 other author(s). (2017)cite arxiv:1709.06102Comment: 17 pages, 7 figures, submitted to MNRAS.Keck Spectroscopy of Faint 3&lt;z&lt;8 Lyman Break Galaxies:- Evidence for a Declining Fraction of Emission Line Sources In the Redshift Range 6&lt;z&lt;8, , , , , , , and . (2011)cite arxiv:1107.1261Comment: 7 pages, 5 figures, submitted to ApJ.The z = 9-10 galaxy population in the Hubble Frontier Fields and CLASH surveys: The z=9 LF and further evidence for a smooth decline in UV luminosity at z >= 8, , and . (2016)cite arxiv:1602.05199Comment: Submitted to MNRAS, 13 pages, 11 figures.