The clustering of typical Ly;1 emitters from z c 2.5–6: Host halo masses depend on Ly;1 and UV luminosities
A.A. Khostovan, D. Sobral, B. Mobasher, J.J. Matthee, R.K. Cochrane, N. Chartab, M. Jafariyazani, A. Paulino-Afonso, S. Santos, J. Calhau, Monthly Notices of the Royal Astronomical Society 489 (2019) 555–573.

The clustering of H ;2 + [OIII] and [OII] emitters since z c 5: Dependencies with line luminosity and stellar mass
A.A. Khostovan, D. Sobral, B. Mobasher, P.N. Best, I. Smail, J.J. Matthee, B. Darvish, H. Nayyeri, S. Hemmati, J.P. Stott, Monthly Notices of the Royal Astronomical Society 478 (2018) 2999–3015.

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.