### Bibliographic note

This is a pre-copy-editing, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The definitive publisher-authenticated version A A Khostovan, D Sobral, B Mobasher, J Matthee, R K Cochrane, N Chartab, M Jafariyazani, A Paulino-Afonso, S Santos, J Calhau, The clustering of typical Ly α emitters from z ∼ 2.5–6: host halo masses depend on Ly α and UV luminosities, Monthly Notices of the Royal Astronomical Society, Volume 489, Issue 1, October 2019, Pages 555–573, https://doi.org/10.1093/mnras/stz2149 is available online at: https://academic.oup.com/mnras/article/489/1/555/5544368