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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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Semi-blind separation of galaxy spectra from a mixture obtained by slitless spectroscopy., , , and . EUSIPCO, page 1641-1645. IEEE, (2015)Galactic Winds with MUSE: A Direct Detection of FeII* Emission from a z = 1.29 Galaxy, , , , , , , , , and 5 other author(s). (2017)cite arxiv:1701.07843Comment: 13 pages, 6 figures, 4 tables, submitted to A&A - comments welcome.Discovery of a 100 kpc-wide ionised gas structure in an over-dense region of the galaxy group COSMOS-Gr30 at z ~ 0.7, , , , , , , , , and 9 other author(s). (2017)cite arxiv:1710.11225Comment: 21 pages, 12 figures, 3 tables, accepted for publication in A&A (27 October 2017).Dark Galaxy Candidates at Redshift ~3.5 Detected with MUSE, , , , , , , , , and 11 other author(s). (2017)cite arxiv:1709.03522Comment: 28 pages, 13 figures, 5 tables, submitted to ApJ.A New Separation Method for Galaxy Spectra Based on Data Fusion between Two Grism Orders in Slitless Spectroscopy., , , , and . ICASSP, page 4245-4249. IEEE, (2019)Separation of galaxy spectra measured with slitless spectroscopy., , , and . Digit. Signal Process., (2020)MUSEQuBES: Calibrating the redshifts of Lyman-\alpha emitters using stacked circumgalactic medium absorption profiles, , , , , , , , , and 10 other author(s). (2019)cite arxiv:1910.03593Comment: 9 Pages, Submitted to MNRAS, Comments Welcome!.The luminosity--metallicity relation in the local Universe from the 2dF Galaxy Redshift Survey, , , , and . Monthly Notices of the Royal Astronomical Society, 350 (2): 396--406 (2004)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 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).