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The VLT SINFONI Mg ii Program for Line Emitters (SIMPLE) II: background quasars probing z $\sim$ 1 galactic winds

, , , , , and . (2015)cite arxiv:1502.07895Comment: 19 pages, 12 figures.

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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.Separation of galaxy spectra measured with slitless spectroscopy., , , and . Digit. Signal Process., (2020)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)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)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.A SINFONI Integral Field Spectroscopy Survey for Galaxy Counterparts to Damped Lyman-alpha Systems - VI. Metallicity and Geometry as Gas Flow Probes, , , , , , , , , and . (2016)cite arxiv:1601.02796Comment: 16 pages, 8 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.