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The MUSE Hubble Ultra Deep Field Survey: IV. Global properties of C III emitters

, , , , , , , , , , , , , , and . (2017)cite arxiv:1710.06432Comment: 16 pages and 13 figures, accepted for publication in A&A.

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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/.MUSE Deep-Fields: The Lya Luminosity Function in the Hubble Deep Field South at 2.91 < z < 6.64, , , , , , , , , and 7 other author(s). (2016)cite arxiv:1609.02920Comment: 13 pages, 8 figures, submitted to MNRAS.The MUSE Hubble Ultra Deep Field Survey VIII : Extended Lyman-alpha haloes around high-redshift star-forming galaxies, , , , , , , , , and 10 other author(s). (2017)cite arxiv:1710.10271Comment: 24 pages, 18 figures, 1 table, accepted for publication in A&A.A stellar census in globular clusters with MUSE: The contribution of rotation to cluster dynamics studied with 200 000 stars, , , , , , , , , and 3 other author(s). (2017)cite arxiv:1710.07257Comment: accepted for publication in MNRAS, 29 pages, 14 figures, radial kinematics profiles available at https://musegc.uni-goettingen.de/.Elevated ionizing photon production efficiency in faint high-equivalent-width Lyman-alpha emitters, , , , , , , , , and 9 other author(s). (2020)cite arxiv:2002.11117Comment: 12 Pages, 6 Figures; Accepted for publication in MNRAS.A young star-forming galaxy at z = 3.5 with an extended Ly\,$\alpha$ halo seen with MUSE, , , , , , , , , and 5 other author(s). (2015)cite arxiv:1512.01212Comment: 19 pages, 15 figures, accepted in MNRAS.MusE GAs FLOw and Wind (MEGAFLOW) I: First MUSE results on background quasars, , , , , , , , , and 6 other author(s). (2016)cite arxiv:1605.03412Comment: 20 pages, 16 figures, submitted to ApJ.The MUSE Hubble Ultra Deep Field Survey: V. Spatially resolved stellar kinematics of galaxies at redshift $0.2z 0.8$, , , , , , , , , and 4 other author(s). (2017)cite arxiv:1710.07694Comment: 25 pages, 27 figures, A&A for accepted (26 June 2017).The MUSE Hubble Ultra Deep Field Survey: IV. Global properties of C III emitters, , , , , , , , , and 5 other author(s). (2017)cite arxiv:1710.06432Comment: 16 pages and 13 figures, accepted for publication in A&A.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.