The clustering of typical Ly α emitters from z ∼ 2.5–6: host halo masses depend on Ly α and UV luminosities
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B. Mobasher | D. Sobral | J. Matthee | S. Santos | A. Paulino-Afonso | J. Calhau | A. A. Khostovan | R. Cochrane | N. Chartab | M. Jafariyazani | A. Khostovan | Nima Chartab Soltani