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No evidence for Population III stars or a Direct Collapse Black Hole in the z = 6.6 Lyman-$\alpha$ emitter 'CR7'

, , , , , , and . (2016)cite arxiv:1609.00727Comment: 10 pages, 5 figures and 1 table. Submitted to MNRAS.

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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.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.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.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.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.COSMOS2020: UV selected galaxies at $z\geq7.5$, , , , , , , , , and 9 other author(s). (2022)cite arxiv:2207.11740Comment: 23 pages, 11 figures, 4 tables, submitted to A&A.The evolution of the galaxy UV luminosity function at redshifts z ~ 8-15 from deep JWST and ground-based near-infrared imaging, , , , , , , , , and 3 other author(s). (2022)cite arxiv:2207.12356Comment: 28 pages, 4 figures in main manuscript, submitted to MNRAS.The SCUBA-2 Cosmology Legacy Survey: the submillimetre properties of Lyman break galaxies at z=3-5, , , , , , , , , and 21 other author(s). (2014)cite arxiv:1407.6712Comment: 12 pages, 8 figures, submitted to MNRAS.On the redshift evolution (0 < z < 4) of dust attenuation and of the total (UV+IR) star formation rate density, , , , , , , , , and 12 other author(s). (2013)cite arxiv:1304.7000Comment: Submitted to A&A.