Confirmation of double peaked Ly;1 emission at z = 6.593: Witnessing a galaxy directly contributing to the reionisation of the universe
J.J. Matthee, D. Sobral, M. Gronke, A. Paulino-Afonso, M. Stefanon, H. Röttgering, Astronomy &; Astrophysics 619 (2018).

The nature of luminous Ly ;1 emitters at z c 2–3: Maximal dust-poor starbursts and highly ionizing AGN
D. Sobral, J.J. Matthee, B. Darvish, I. Smail, P.N. Best, L. Alegre, H. Röttgering, B. Mobasher, A. Paulino-Afonso, A. Stroe, I. Oteo, Monthly Notices of the Royal Astronomical Society 477 (2018) 2817–2840.

Slicing COSMOS with SK: The evolution of typical Ly;1 emitters and the Ly;1 escape fraction from z c 2 to 6
D. Sobral, S. Santos, J.J. Matthee, A. Paulino-Afonso, B. Ribeiro, J. Calhau, A.A. Khostovan, Monthly Notices of the Royal Astronomical Society 476 (2018) 4725–4752.

Kiloparsec-scale gaseous clumps and star formation at z = 5–7
S. Carniani, R. Maiolino, R. Amorin, L. Pentericci, A. Pallottini, A. Ferrara, C.J. Willott, R. Smit, J.J. Matthee, D. Sobral, P. Santini, M. Castellano, S. De Barros, A. Fontana, A. Grazian, L. Guaita, Monthly Notices of the Royal Astronomical Society 478 (2018) 1170–1184.

Star-forming galaxies are predicted to lie on a fundamental plane of mass, star formation rate, and ;1-enhancement
J.J. Matthee, J. Schaye, Monthly Notices of the Royal Astronomical Society: Letters 479 (2018) L34–L39.