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Evolution of the dust emission of massive galaxies up to z=4 and constraints on their dominant mode of star formation

, , , , , , , , , , , , , , , , , , , and . (2014)cite arxiv:1409.5796Comment: 17 pages, 14 figures, 2 tables, submitted to A&A.

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The 0.1<z<1.65 evolution of the bright end of the OII luminosity function, , , , , , , , , and 26 other author(s). (2014)cite arxiv:1408.1523Comment: 20 pages, 22 Figures, submitted.Evolution of the dust emission of massive galaxies up to z=4 and constraints on their dominant mode of star formation, , , , , , , , , and 10 other author(s). (2014)cite arxiv:1409.5796Comment: 17 pages, 14 figures, 2 tables, submitted to A&A.Predictions for the CO emission of galaxies from a coupled simulation of galaxy formation and photon dominated regions, , , , , , and . (2012)cite arxiv:1204.0795Comment: 23 pages, 13 figures. Submitted to MNRAS.Determining the systemic redshift of Lyman-\alpha emitters with neural networks and improving the measured large-scale clustering, , , , , and . (2020)cite arxiv:2005.12931Comment: 22 Pages, 20 figures, a lot of fun.Lyman-alpha emitters in a cosmological volume II: the impact of the intergalactic medium, , , , , and . (2019)cite arxiv:1904.04274Comment: 25 pages, 18 figures , a lot of love.Numerical overcooling in shocks, , , and . (2011)cite arxiv:1106.0306Comment: 16 pages, 11 figures, accepted into MNRAS.Can galactic outflows explain the properties of Ly-alpha emitters?, , and . (2011)cite arxiv:1110.5701 Comment: 28 pages, 21 figures, submitted to MNRAS.Cosmic evolution of the atomic and molecular gas content of galaxies, , , , , and . (2011)cite arxiv:1105.2294 Comment: 17 pages, 16 figures. Submitted to MNRAS. Comments are welcome.