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The first low-mass stars: critical metallicity or dust-to-gas ratio?

, , , and . (2011)cite arxiv:1109.2900 Comment: accepted by MNRAS, 12 pages, 8 figures.

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Faint progenitors of luminous $z 6$ quasars: why don't we see them?, , , , , and . (2016)cite arxiv:1612.04188Comment: 12 pages, 9 figures, accepted for publication in MNRAS.The first low-mass stars: critical metallicity or dust-to-gas ratio?, , , and . (2011)cite arxiv:1109.2900 Comment: accepted by MNRAS, 12 pages, 8 figures.The formation of the extremely primitive star SDSS J102915+172927 relies on dust, , , , , , and . (2012)cite arxiv:1203.4234Comment: 5 pages, 3 figures, accepted as a Letter to MNRAS.The spectral energy distribution of z ~ 6 quasars: the case of SDSS J1148+5251, , , , and . (2014)cite arxiv:1402.2279Comment: Submitted to MNRAS in the present form on October 4th 2013. Still waiting for the first referee report. Comments are welcome.The dust content of the most metal-poor star-forming galaxies, , and . (2016)cite arxiv:1601.01686Comment: 10 pages, 5 figures, to appear in MNRAS.On the Stellar Populations of Galaxies at z=9-11: The Growth of Metals and Stellar Mass at Early Times, , , , , , , , , and 11 other author(s). (2021)cite arxiv:2111.05351Comment: 27 pages + Appendix; Submitted to ApJ; Comments welcome.Multi-flavour SMBH seeding and evolution in cosmological environments, , , , and . (2022)cite arxiv:2203.13846Comment: 22 pages, 13 figures, submitted to MNRAS.Reionization with galaxies and active galactic nuclei, , , , , , , , and . (2020)cite arxiv:2001.06021Comment: Submitted to MNRAS; comments welcome.Molecular gas on large circumgalactic scales at z=3.47, , , , , , , , , and 2 other author(s). (2016)cite arxiv:1611.07026Comment: 17 pages, 16 figures; submitted to MNRAS; comments are welcome.Where does galactic dust come from?, , , , , , , and . (2017)cite arxiv:1707.05328Comment: 6 pages, 4 figures, submitted to MNRAS, comments are welcome.