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Ionising the Intergalactic Medium by Star Clusters ? The first empirical evidence

, , , , , , , , , , , , , , , , and . (2019)cite arxiv:1904.07941Comment: 9 pages, 6 figures and 1 table, submitted to MNRAS. Comments welcome.

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The evolution of neutral gas in damped Lyman $\alpha$ systems from the XQ-100 survey, , , , , , , , , and 3 other author(s). (2015)cite arxiv:1511.05003Comment: Submitted to MNRAS, this version follows the referee's report and minor revisions. Large tables are included in the source file tarball.Direct Lyman continuum and Lyman-alpha escape observed at redshift 4, , , , , , , , , and 9 other author(s). (2017)cite arxiv:1712.07661Comment: 5 pages, 4 figures, 1 table, Submitted to MNRAS, Comments Welcome.Solving the conundrum of intervening strong MgII absorbers towards GRBs and quasars, , , , , , , , , and 26 other author(s). (2017)cite arxiv:1709.01084Comment: 10 pages, accepted for publication in A&A.Ionising the Intergalactic Medium by Star Clusters ? The first empirical evidence, , , , , , , , , and 7 other author(s). (2019)cite arxiv:1904.07941Comment: 9 pages, 6 figures and 1 table, submitted to MNRAS. Comments welcome.The Luminosity Function of bright QSOs at z~4 and implications for the cosmic ionizing background, , , , , , , , , and 1 other author(s). (2021)cite arxiv:2103.10446Comment: Accepted for publication in ApJ, 15 pages, 5 figures, 4 tables.XQ-100: A legacy survey of one hundred 3.5 z < 4.5 quasars observed with VLT/XSHOOTER, , , , , , , , , and 16 other author(s). (2016)cite arxiv:1607.08776Comment: In press at A&A.Exploring the Thermal State of the Low-Density Intergalactic Medium at z=3 with an Ultra-High Signal-to-Noise QSO Spectrum, , , , , , , , , and 4 other author(s). (2016)cite arxiv:1611.03805Comment: Accepted for publication on MNRAS.Metals in the z~3 intergalactic medium: results from an ultra-high signal-to-noise ratio UVES quasar spectrum, , , , , , , , , and 6 other author(s). (2016)cite arxiv:1608.06116Comment: 23 pages, 28 figures. Submitted to MNRAS (revised version after first referee report).High-resolution spectroscopy at the faintest limits: an "ELT-like" spectrum of a young optically-thin L=0.02L* star-forming galaxy at z=3.12, , , , , , , , , and 22 other author(s). (2016)cite arxiv:1603.01616Comment: 7 pages, 4 figures and 1 table; ApJL submitted.On the AGN nature of two UV bright sources at z_spec~5.5 in the CANDELS fields: an update of the AGN space density at M1450~-22.5, , , , , , , , , and 1 other author(s). (2020)cite arxiv:2006.02451Comment: Accepted for publication in ApJ. 21 pages, 6 figures, 4 tables.