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Equivalent widths of Lyman $\alpha$ emitters in MUSE-Wide and MUSE-Deep, , , , , , , , , and 8 other author(s). (2022)cite arxiv:2202.06642Comment: 28 pages, 21 + 1 figures, 7 + 1 tables, accepted for publication in A&A.MUSE-inspired view of the quasar Q2059-360, its Lyman alpha blob, and its neighborhood, , , , , , , , and . (2017)cite arxiv:1705.05728Comment: Accepted for publication in Astronomy & Astrophysics; 16 pages, 19 figures.The MUSE Hubble Ultra Deep Field Survey: III. Testing photometric redshifts to 30th magnitude, , , , , , , , , and 7 other author(s). (2017)cite arxiv:1710.05062Comment: 24 pages and 25 figures, accepted for A&A.MUSE observations of the lensing cluster Abell 1689, , , , , , , , , and 7 other author(s). (2016)cite arxiv:1603.05833Comment: 12 pages, 11 figures.High-resolution spectroscopy at the faintest limits: an "ELT-like" spectrum of a young optically-thin L=0.02L* star-forming galaxy at z=3.12, , , , , , , , , and 22 other author(s). (2016)cite arxiv:1603.01616Comment: 7 pages, 4 figures and 1 table; ApJL submitted.Ly\alpha-Lyman Continuum connection in 3.5 < z < 4.3 star-forming galaxies from the VUDS survey, , , , , , , , , and 9 other author(s). (2017)cite arxiv:1710.10184Comment: submitted to A&A.An extreme OIII emitter at $z=3.2$: a low metallicity Lyman continuum source, , , , , , , , , and 9 other author(s). (2015)cite arxiv:1507.06648Comment: 13 pages, 10 figures, submitted to A&A. Comments welcome.Lyman-alpha blobs: polarization arising from cold accretion, , , and . (2016)cite arxiv:1604.02066Comment: 14 pages, 9 figures (+4 in appendices). Accepted for publication in Astronomy & Astrophysics.Extended Lyman alpha haloes around individual high-redshift galaxies revealed by MUSE, , , , , , , , , and 15 other author(s). (2015)cite arxiv:1509.05143Comment: submitted to Astronomy & Astrophysics.The VIMOS Ultra Deep Survey: The role of HI kinematics and HI column density on the escape of Lyalpha photons in star-forming galaxies at 2<z<4, , , , , , , , , and 15 other author(s). (2017)cite arxiv:1707.01443Comment: Accepted on May 2017.