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Chasing passive galaxies in the early Universe: a critical analysis in CANDELS GOODS-South

, , , , , , , , , , , , , , and . (2017)cite arxiv:1709.00429Comment: 28 pages, 13 figures, 2 tables.

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Constraining Lyman-alpha spatial offsets at $3<z<5.5$ from VANDELS slit spectroscopy, , , , , , , , , and 12 other author(s). (2019)cite arxiv:1905.09467Comment: Submitted to MNRAS.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.MOONS: a multi-object optical and near-infrared spectrograph for the VLT, , , , , , , , , and 70 other author(s). Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, volume 8446 of Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, (September 2012)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.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.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.The bright end of the galaxy luminosity function at z ~ 7: before the onset of mass quenching?, , , , , , , , , and 2 other author(s). (2013)cite arxiv:1312.5643Comment: 35 pages, 13 figures, submitted to MNRAS.No evidence for a significant AGN contribution to cosmic hydrogen reionization, , and . (2017)cite arxiv:1704.07750Comment: 20 pages, 8 figures, submitted to MNRAS.The properties of He II 1640 emitters at z ~ 2.5-5 from the VANDELS survey, , , , , , , , , and 16 other author(s). (2019)cite arxiv:1911.09999Comment: 19 pages, 10 figures (including appendix), submitted to A&A. Comments welcome!.