Matthee, J. J. (2021). Differences in galaxy colours are not just about the mass. Nature Astronomy. Springer Nature.https://doi.org/10.1038/s41550-021-01415-y 

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 

Calhau, J., Sobral, D., Santos, S., Matthee, J. J., Paulino-Afonso, A., Stroe, A.,https://doi.org/10.1093/mnras/staa476__Adams, B. (2020). The X-ray and radio activity of typical and luminous Ly;1 emitters from z c 2 to z c 6: Evidence for a diverse, evolving population. Monthly Notices of the Royal Astronomical Society. Oxford University Press.https://doi.org/10.1093/mnras/staa476 

Nanayakkara, T., Brinchmann, J., Boogaard, L., Bouwens, R., Cantalupo, S., Feltre, A.,https://doi.org/10.1051/0004-6361/201834565__Verhamme, A. (2019). Exploring HefII;b1640 emission line properties at z c24. Astronomy &; Astrophysics. EDP Sciences.https://doi.org/10.1051/0004-6361/201834565 

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 

Khostovan, A. A., Sobral, D., Mobasher, B., Matthee, J. J., Cochrane, R. K., Chartab, N.,https://doi.org/10.1093/mnras/stz2149__Calhau, J. (2019). The clustering of typical Ly;1 emitters from z c 2.5–6: Host halo masses depend on Ly;1 and UV luminosities. Monthly Notices of the Royal Astronomical Society. Oxford University Press.https://doi.org/10.1093/mnras/stz2149 

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 

Khostovan, A. A., Sobral, D., Mobasher, B., Best, P. N., Smail, I., Matthee, J. J.,https://doi.org/10.1093/mnras/sty925__Stott, J. P. (2018). The clustering of H ;2 + [OIII] and [OII] emitters since z c 5: Dependencies with line luminosity and stellar mass. Monthly Notices of the Royal Astronomical Society. Oxford University Press.https://doi.org/10.1093/mnras/sty925 

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 

Stroe, A., Sobral, D., Matthee, J. J., Calhau, J., &; Oteo, I. (2017). A 1.4 de blind survey for C II], C III] and C IV at z c 0.7–1.5 – I. Nature, morphologies and equivalent widths . Monthly Notices of the Royal Astronomical Society. Oxford University Press.https://doi.org/10.1093/mnras/stx1712 

Stroe, A., Sobral, D., Matthee, J. J., Calhau, J., &; Oteo, I. (2017). A 1.4 de blind survey for C II], C III] and C IV at z c 0.7–1.5 – II. Luminosity functions and cosmic average line ratios. Monthly Notices of the Royal Astronomical Society. Oxford University Press.https://doi.org/10.1093/mnras/stx1713 

Matthee, J. J., Sobral, D., Best, P., Smail, I., Bian, F., Darvish, B.,https://doi.org/10.1093/mnras/stx1569__Fan, X. (2017). Boötes-HiZELS: An optical to near-infrared survey of emission-line galaxies at z = 0.4–4.7. Monthly Notices of the Royal Astronomical Society. Oxford University Press.https://doi.org/10.1093/mnras/stx1569