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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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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.Angular momentum evolution of galaxies over the past 10-Gyr: A MUSE and KMOS dynamical survey of 400 star-forming galaxies from z=0.3-1.7, , , , , , , , , and 16 other author(s). (2017)cite arxiv:1701.07448Comment: MNRAS in press. 21 pages; 12 figures. The full pdf, which includes an additional 32 pages of supplementary figures and data tables are available from http://astro.dur.ac.uk/~ams/MUSEcubes/.The distribution of atomic hydrogen in EAGLE galaxies: morphologies, profiles, and HI holes, , , , , , , , , and 1 other author(s). (2015)cite arxiv:1511.04909Comment: 23 pages, 17 figures (16 pages, 9 figures without appendices), accepted by MNRAS.The Taipan Galaxy Survey: Scientific Goals and Observing Strategy, , , , , , , , , and 30 other author(s). (2017)cite arxiv:1706.01246Comment: Submitted to PASA; 28 pages, 17 figures, 2 tables.X-shooter Spectroscopy and HST Imaging of 15 Ultra Massive Quiescent Galaxies at $z\gtrsim2$, , , , , , , , , and 16 other author(s). (2019)cite arxiv:1912.01619Comment: 30 pages, 10 figures, accepted in ApJ.The cosmic radio background from 150 MHz--8.4 GHz, and its division into AGN and star-forming galaxy flux, , , , , , and . (2023)cite arxiv:2301.03699.An accurate low-redshift measurement of the cosmic neutral hydrogen density, , , , , , , , , and . (2019)cite arxiv:1907.10375Comment: 17 pages, 24 figures.On the evolution of the molecular gas fraction of star forming galaxies, , , , , and . (2011)cite arxiv:1102.3694 Comment: Accepted for publication in ApJ Letters; 5 pages, 2 figures.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.Multi-wavelength consensus of large-scale linear bias, , , , , , and . (2019)cite arxiv:1909.12069Comment: 19 pages, submitted to MNRAS.