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 
LibreCat: https://research-explorer.ista.ac.at/record/11535
DOI: 10.1093/mnras/stz2149
arXiv: 1811.00556

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 
LibreCat: https://research-explorer.ista.ac.at/record/11549
DOI: 10.1093/mnras/sty925
arXiv: 1705.01101

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