Kusakabe, H., Verhamme, A., Blaizot, J., Garel, T., Wisotzki, L., Leclercq, F.,https://doi.org/10.1051/0004-6361/202142302__Vitte, E. (2022). The MUSE eXtremely Deep Field: Individual detections of Ly;1 haloes around rest-frame UV-selected galaxies at zhttps://doi.org/10.1051/0004-6361/202142302__2.9–4.4. Astronomy &; Astrophysics. EDP Sciences.https://doi.org/10.1051/0004-6361/202142302 

Kerutt, J., Wisotzki, L., Verhamme, A., Schmidt, K. B., Leclercq, F., Herenz, E. C.,https://doi.org/10.1051/0004-6361/202141900__Vitte, E. (2022). Equivalent widths of Lyman ;1 emitters in MUSE-Wide and MUSE-Deep. Astronomy &; Astrophysics. EDP Sciences.https://doi.org/10.1051/0004-6361/202141900 

Matthee, J. J., Feltre, A., Maseda, M., Nanayakkara, T., Boogaard, L., Bacon, R.,https://doi.org/10.1051/0004-6361/202142187__Wisotzki, L. (2022). Deciphering stellar metallicities in the early universe: Case study of a young galaxy at z = 4.77 in the MUSE eXtremely Deep Field. Astronomy &; Astrophysics. EDP Sciences.https://doi.org/10.1051/0004-6361/202142187 

Matthee, J. J., Sobral, D., Hayes, M., Pezzulli, G., Gronke, M., Schaerer, D.,https://doi.org/10.1093/mnras/stab1304__Amorín, R. (2021). The X-SHOOTER Lyman ;1 survey at z = 2 (XLS-z2) I: What makes a galaxy a Lyman ;1 emitter? Monthly Notices of the Royal Astronomical Society. Oxford University Press.https://doi.org/10.1093/mnras/stab1304 

Gronke, M., Ocvirk, P., Mason, C., Matthee, J. J., Bosman, S. E. I., Sorce, J. G.,https://doi.org/10.1093/mnras/stab2762__Yepes, G. (2021). Lyman-;1 transmission properties of the intergalactic medium in the CoDaII simulation. Monthly Notices of the Royal Astronomical Society. Oxford University Press.https://doi.org/10.1093/mnras/stab2762 

Leclercq, F., Bacon, R., Verhamme, A., Garel, T., Blaizot, J., Brinchmann, J.,https://doi.org/10.1051/0004-6361/201937339__Wisotzki, L. (2020). The MUSE Hubble Ultra Deep field survey: XIII. Spatially resolved spectral properties of Lyman ;1 haloes around star-forming galaxies at z &; 3. Astronomy &; Astrophysics. EDP Sciences.https://doi.org/10.1051/0004-6361/201937339 

Santos, S., Sobral, D., Matthee, J. J., Calhau, J., da Cunha, E., Ribeiro, B.,https://doi.org/10.1093/mnras/staa093__Butterworth, J. (2020). The evolution of rest-frame UV properties, Ly;1 EWs, and the SFR–stellar mass relation at z c 2–6 for SK LAEs. Monthly Notices of the Royal Astronomical Society. Oxford University Press.https://doi.org/10.1093/mnras/staa093 

Matthee, J. J., &; Sobral, D. (2020). Unveiling the most luminous Lyman-;1 emitters in the epoch of reionisation. In Proceedings of the International Astronomical Union (Vol. 15, pp. 21–25). Cambridge University Press.https://doi.org/10.1017/s1743921319009451 

Sobral, D., &; Matthee, J. J. (2019). Predicting Ly;1 escape fractions with a simple observable: Ly;1 in emission as an empirically calibrated star formation rate indicator. Astronomy &; Astrophysics. EDP Sciences.https://doi.org/10.1051/0004-6361/201833075 

Matthee, J. J., &; Schaye, J. (2019). The origin of scatter in the star formation rate–stellar mass relation. Monthly Notices of the Royal Astronomical Society. Oxford University Press.https://doi.org/10.1093/mnras/stz030 

Matthee, J. J., Sobral, D., Gronke, M., Paulino-Afonso, A., Stefanon, M., &; Röttgering, H. (2018). Confirmation of double peaked Ly;1 emission at z = 6.593: Witnessing a galaxy directly contributing to the reionisation of the universe. Astronomy &; Astrophysics. EDP Sciences.https://doi.org/10.1051/0004-6361/201833528 

Sobral, D., Santos, S., Matthee, J. J., Paulino-Afonso, A., Ribeiro, B., Calhau, J., &; Khostovan, A. A. (2018). Slicing COSMOS with SK: The evolution of typical Ly;1 emitters and the Ly;1 escape fraction from z c 2 to 6. Monthly Notices of the Royal Astronomical Society. Oxford University Press.https://doi.org/10.1093/mnras/sty378 

Carniani, S., Maiolino, R., Amorin, R., Pentericci, L., Pallottini, A., Ferrara, A.,https://doi.org/10.1093/mnras/sty1088__Guaita, L. (2018). Kiloparsec-scale gaseous clumps and star formation at z = 5–7. Monthly Notices of the Royal Astronomical Society. Oxford University Press.https://doi.org/10.1093/mnras/sty1088 

Matthee, J. J., &; Schaye, J. (2018). Star-forming galaxies are predicted to lie on a fundamental plane of mass, star formation rate, and ;1-enhancement. Monthly Notices of the Royal Astronomical Society: Letters. Oxford University Press.https://doi.org/10.1093/mnrasl/sly093 

Matthee, J. J., Sobral, D., Boone, F., Röttgering, H., Schaerer, D., Girard, M.,https://doi.org/10.3847/1538-4357/aa9931__Mobasher, B. (2017). ALMA reveals metals yet no dust within multiple components in C. The Astrophysical Journal. IOP Publishing.https://doi.org/10.3847/1538-4357/aa9931 

Matthee, J. J., Schaye, J., Crain, R. A., Schaller, M., Bower, R., &; Theuns, T. (2017). The origin of scatter in the stellar mass–halo mass relation of central galaxies in the EAGLE simulation. Monthly Notices of the Royal Astronomical Society. Oxford University Press.https://doi.org/10.1093/mnras/stw2884 

Lagos, C. del P., Theuns, T., Schaye, J., Furlong, M., Bower, R. G., Schaller, M.,https://doi.org/10.1093/mnras/stw717__Matthee, J. J. (2016). The Fundamental Plane of star formation in galaxies revealed by the EAGLE hydrodynamical simulations. Monthly Notices of the Royal Astronomical Society. Oxford University Press.https://doi.org/10.1093/mnras/stw717 

Sobral, D., Matthee, J. J., Best, P. N., Smail, I., Khostovan, A. A., Milvang-Jensen, B.,https://doi.org/10.1093/mnras/stv1076__Mobasher, B. (2015). CF-HiZELS, an c10 de emission-line survey with spectroscopic follow-up: H;1, [OIII] + H;2 and [OII] luminosity functions at z = 0.8, 1.4 and 2.2 . Monthly Notices of the Royal Astronomical Society. Oxford University Press.https://doi.org/10.1093/mnras/stv1076