Khostovan, A. A., et al. “The Clustering of Typical Ly;1 Emitters from z c 2.5–6: Host Halo Masses Depend on Ly;1 and UV Luminosities.”10.1093/mnras/stz2149__Monthly Notices of the Royal Astronomical Society, vol. 489, no. 1, Oxford University Press, 2019, pp. 555–73, doi:10.1093/mnras/stz2149.
LibreCat: https://research-explorer.ista.ac.at/record/11535
DOI: 10.1093/mnras/stz2149
arXiv: 1811.00556

Khostovan, A. A., et al. “The Clustering of H ;2 + [OIII] and [OII] Emitters since z c 5: Dependencies with Line Luminosity and Stellar Mass.”10.1093/mnras/sty925__Monthly Notices of the Royal Astronomical Society, vol. 478, no. 3, Oxford University Press, 2018, pp. 2999–3015, doi:10.1093/mnras/sty925.
LibreCat: https://research-explorer.ista.ac.at/record/11549
DOI: 10.1093/mnras/sty925
arXiv: 1705.01101

Sobral, D., et al. “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 .”10.1093/mnras/stv1076__Monthly Notices of the Royal Astronomical Society, vol. 451, no. 3, Oxford University Press, 2015, pp. 2303–23, doi:10.1093/mnras/stv1076.
LibreCat: https://research-explorer.ista.ac.at/record/11580
DOI: 10.1093/mnras/stv1076
arXiv: 1502.06602