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The MUSE Hubble Ultra Deep Field Survey: V. Spatially resolved stellar kinematics of galaxies at redshift $0.2z 0.8$

, , , , , , , , , , , , , и . (2017)cite arxiv:1710.07694Comment: 25 pages, 27 figures, A&A for accepted (26 June 2017).

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Bernhard Bouché

Eva Bouché

Elisabeth Bouché

Winfried Bouché

Thomas Bouché

 

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A SINFONI Integral Field Spectroscopy Survey for Galaxy Counterparts to Damped Lyman-alpha Systems - III. Three Additional Detections, , , , и . (2011)cite arxiv:1110.0666Comment: 16 pages, 8 figures, accepted for publication in MNRAS.Searching for Light in the Darkness: Bounds on ALP Dark Matter with the optical MUSE-Faint survey, , , , , , и . (2020)cite arxiv:2009.01310Comment: 11 pages, 5 figures.Optical pancreatic beta cell based biosensor, applications and glucose monitoring., , , , , и . IEEE SENSORS, стр. 1-4. IEEE, (2019)An adaptable and personalized web telecommunication model., , и . Bell Labs Tech. J., 16 (1): 3-17 (2011)Shocked Superwinds from the z~2 Clumpy Star-forming Galaxy, ZC406690, , , , , , , , , и 13 other автор(ы). (2012)cite arxiv:1204.4727Comment: 21 pages, 7 figures, Accepted for publication in ApJ.The VLT SINFONI Mg ii Program for Line Emitters (SIMPLE) II: background quasars probing z $\sim$ 1 galactic winds, , , , , и . (2015)cite arxiv:1502.07895Comment: 19 pages, 12 figures.MusE GAs FLOw and Wind (MEGAFLOW) I: First MUSE results on background quasars, , , , , , , , , и 6 other автор(ы). (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 $0.2z 0.8$, , , , , , , , , и 4 other автор(ы). (2017)cite arxiv:1710.07694Comment: 25 pages, 27 figures, A&A for accepted (26 June 2017).MUSEQuBES: Calibrating the redshifts of Lyman-\alpha emitters using stacked circumgalactic medium absorption profiles, , , , , , , , , и 10 other автор(ы). (2019)cite arxiv:1910.03593Comment: 9 Pages, Submitted to MNRAS, Comments Welcome!.Ubiquitous giant Lyman $\alpha$ nebulae around the brightest quasars at $z\sim3.5$ revealed with MUSE, , , , , , , , , и 10 other автор(ы). (2016)cite arxiv:1605.01422Comment: 19 pages, 8 figures, 3 Tables, submitted to ApJ.