The Ly;1 luminosity function at z= 5.7–6.6 and the steep drop of the faint end: Implications for reionization
S. Santos, D. Sobral, J.J. Matthee, Monthly Notices of the Royal Astronomical Society 463 (2016) 1678–1691.
LibreCat: https://research-explorer.ista.ac.at/record/11574
DOI: 10.1093/mnras/stw2076
arXiv: 1606.07435

The most luminous H ;1 emitters at z c 0.8–2.23 from HiZELS: Evolution of AGN and star-forming galaxies
D. Sobral, S.A. Kohn, P.N. Best, I. Smail, C.M. Harrison, J. Stott, J. Calhau, J.J. Matthee, Monthly Notices of the Royal Astronomical Society 457 (2016) 1739–1752.
LibreCat: https://research-explorer.ista.ac.at/record/11576
DOI: 10.1093/mnras/stw022
arXiv: 1601.02266

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.
LibreCat: https://research-explorer.ista.ac.at/record/11575
DOI: 10.1093/mnras/stw717
arXiv: 1510.08067

The CALYMHA survey: Ly;1 escape fraction and its dependence on galaxy properties at z = 2.23
J.J. Matthee, D. Sobral, I. Oteo, P. Best, I. Smail, H. Röttgering, A. Paulino-Afonso, Monthly Notices of the Royal Astronomical Society 458 (2016) 449–467.
LibreCat: https://research-explorer.ista.ac.at/record/11578
DOI: 10.1093/mnras/stw322
arXiv: 1602.02756

Using galaxy formation simulations to optimize LIGO follow-up observations
E. Antolini, I. Caiazzo, R. Davé, J.S. Heyl, Monthly Notices of the Royal Astronomical Society 466 (2016) 2212–2216.
LibreCat: https://research-explorer.ista.ac.at/record/15242
DOI: 10.1093/mnras/stw3292
arXiv: 1612.04412

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.
LibreCat: https://research-explorer.ista.ac.at/record/11580
DOI: 10.1093/mnras/stv1076
arXiv: 1502.06602

Identification of the brightest Ly;1 emitters at z = 6.6: implications for the evolution of the luminosity function in the reionization era
J.J. Matthee, D. Sobral, S. Santos, H. Röttgering, B. Darvish, B. Mobasher, Monthly Notices of the Royal Astronomical Society 451 (2015) 400–417.
LibreCat: https://research-explorer.ista.ac.at/record/11581
DOI: 10.1093/mnras/stv947
arXiv: 1502.07355

The brightest Ly;1 emitter: Pop III or black hole?
A. Pallottini, A. Ferrara, F. Pacucci, S. Gallerani, S. Salvadori, R. Schneider, D. Schaerer, D. Sobral, J.J. Matthee, Monthly Notices of the Royal Astronomical Society 453 (2015) 2465–2470.
LibreCat: https://research-explorer.ista.ac.at/record/11579
DOI: 10.1093/mnras/stv1795
arXiv: 1506.07173

A 10 de Lyman ;1 survey at z=8.8 with spectroscopic follow-up: Strong constraints on the luminosity function and implications for other surveys
J.J. Matthee, D. Sobral, A.M. Swinbank, I. Smail, P.N. Best, J.-W. Kim, M. Franx, B. Milvang-Jensen, J. Fynbo, Monthly Notices of the Royal Astronomical Society 440 (2014) 2375–2387.
LibreCat: https://research-explorer.ista.ac.at/record/11583
DOI: 10.1093/mnras/stu392
arXiv: 1402.6697

A relationship between specific star formation rate and metallicity gradient within z c 1 galaxies from KMOS-HiZELS
J.P. Stott, D. Sobral, A.M. Swinbank, I. Smail, R. Bower, P.N. Best, R.M. Sharples, J.E. Geach, J.J. Matthee, Monthly Notices of the Royal Astronomical Society 443 (2014) 2695–2704.
LibreCat: https://research-explorer.ista.ac.at/record/11582
DOI: 10.1093/mnras/stu1343
arXiv: 1407.1047