The MUSE Hubble Ultra Deep field survey: XIII. Spatially resolved spectral properties of Lyman ;1 haloes around star-forming galaxies at z > 3
F. Leclercq, R. Bacon, A. Verhamme, T. Garel, J. Blaizot, J. Brinchmann, S. Cantalupo, A. Claeyssens, S. Conseil, T. Contini, T. Hashimoto, E.C. Herenz, H. Kusakabe, R.A. Marino, M. Maseda, J.J. Matthee, P. Mitchell, G. Pezzulli, J. Richard, K.B. Schmidt, L. Wisotzki, Astronomy &; Astrophysics 635 (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
S. Santos, D. Sobral, J.J. Matthee, J. Calhau, E. da Cunha, B. Ribeiro, A. Paulino-Afonso, P. Arrabal Haro, J. Butterworth, Monthly Notices of the Royal Astronomical Society 493 (2020) 141–160.

Unveiling the most luminous Lyman-;1 emitters in the epoch of reionisation
J.J. Matthee, D. Sobral, in:, Proceedings of the International Astronomical Union, Cambridge University Press, 2020, pp. 21–25.

Predicting Ly;1 escape fractions with a simple observable: Ly;1 in emission as an empirically calibrated star formation rate indicator
D. Sobral, J.J. Matthee, Astronomy &; Astrophysics 623 (2019).

The origin of scatter in the star formation rate–stellar mass relation
J.J. Matthee, J. Schaye, Monthly Notices of the Royal Astronomical Society 484 (2019) 915–932.

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).

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.

ALMA reveals metals yet no dust within multiple components in C
J.J. Matthee, D. Sobral, F. Boone, H. Röttgering, D. Schaerer, M. Girard, A. Pallottini, L. Vallini, A. Ferrara, B. Darvish, B. Mobasher, The Astrophysical Journal 851 (2017).

The origin of scatter in the stellar mass–halo mass relation of central galaxies in the EAGLE simulation
J.J. Matthee, J. Schaye, R.A. Crain, M. Schaller, R. Bower, T. Theuns, Monthly Notices of the Royal Astronomical Society 465 (2017) 2381–2396.

The Fundamental Plane of star formation in galaxies revealed by the EAGLE hydrodynamical simulations
C. del P. Lagos, T. Theuns, J. Schaye, M. Furlong, R.G. Bower, M. Schaller, R.A. Crain, J.W. Trayford, J.J. Matthee, Monthly Notices of the Royal Astronomical Society 459 (2016) 2632–2650.

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 
D. Sobral, J.J. Matthee, P.N. Best, I. Smail, A.A. Khostovan, B. Milvang-Jensen, J.-W. Kim, J. Stott, J. Calhau, H. Nayyeri, B. Mobasher, Monthly Notices of the Royal Astronomical Society 451 (2015) 2303–2323.