The MUSE Hubble Ultra Deep Field Survey. XIV. Evolution of the Ly α emitter fraction from z = 3 to z = 6

Author(s):: Kusakabe, H.; Blaizot, J.; Garel, T.; Verhamme, A.; Bacon, R.; Richard, J.; Hashimoto, T.; Inami, H.; Conseil, S.; Guiderdoni, B.; Drake, A.B.; Christian Herenz, E.; Schaye, J. (0000-0002-0668-5560); Oesch, P.; Matthee, J.; Anna Marino, R.; Borello Schmidt, K.; Pelló, R.; Maseda, M.V. (0000-0003-0695-4414); Leclercq, F.; Kerutt, J.; Mahler, G.

Published: 2020
Publication type: Article / Letter to editor

Date issued: 2020-06-03
Language: English
Is part of: Astronomy & Astrophysics (2020), Vol. 638, p. A12
hdl: 1887/3134410
doi: 10.1051/0004-6361/201937340
URL: https://ui.adsabs.harvard.edu/abs/2020A&A...638A..12K