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Multi-flavour SMBH seeding and evolution in cosmological environments

, , , , and . (2022)cite arxiv:2203.13846Comment: 22 pages, 13 figures, submitted to MNRAS.

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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.Multi-flavour SMBH seeding and evolution in cosmological environments, , , , and . (2022)cite arxiv:2203.13846Comment: 22 pages, 13 figures, submitted to MNRAS.Where does galactic dust come from?, , , , , , , and . (2017)cite arxiv:1707.05328Comment: 6 pages, 4 figures, submitted to MNRAS, comments are welcome.The low-end of the black hole mass function at cosmic dawn, , , , , and . (2022)cite arxiv:2201.02630Comment: 26 pages, 13 figures, 1 table. Accepted for publication in MNRAS.Astrophysics with the Laser Interferometer Space Antenna, , , , , , , , , and 145 other author(s). (2022)cite arxiv:2203.06016Comment: submitted to Living Reviews In Relativity.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.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.