Kusakabe H, Blaizot J, Garel T, et al. The MUSE Hubble Ultra Deep Field Survey: XIV. Evolution of the Ly;1 emitter fraction from z = 3 to z = 6. Astronomy &; Astrophysics. 2020;638. doi:10.1051/0004-6361/201937340
LibreCat: https://research-explorer.ista.ac.at/record/11503
DOI: 10.1051/0004-6361/201937340
arXiv: 2003.12083

Feltre A, Maseda MV, Bacon R, et al. The MUSE Hubble Ultra Deep Field Survey: XV. The mean rest-UV spectra of Ly;1 emitters at z &; 3. Astronomy &; Astrophysics. 2020;641. doi:10.1051/0004-6361/202038133
LibreCat: https://research-explorer.ista.ac.at/record/11501
DOI: 10.1051/0004-6361/202038133
arXiv: 2007.01878

Nanayakkara T, Brinchmann J, Boogaard L, et al. Exploring HefII;b1640 emission line properties at z c24. Astronomy &; Astrophysics. 2019;648. doi:10.1051/0004-6361/201834565
LibreCat: https://research-explorer.ista.ac.at/record/11499
DOI: 10.1051/0004-6361/201834565
arXiv: 1902.05960

Matthee JJ, Sobral D, Darvish B, et al. Spectroscopic properties of luminous Ly;1 emitters at z10.1093/mnras/stx2061__6–7 and comparison to the Lyman-break population. Monthly Notices of the Royal Astronomical Society. 2017;472(1):772-787. doi:10.1093/mnras/stx2061
LibreCat: https://research-explorer.ista.ac.at/record/11572
DOI: 10.1093/mnras/stx2061
arXiv: 1706.06591