The clustering of H β + [O III] and [O II] emitters since z ∼ 5: dependencies with line luminosity and stellar mass
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I. Smail | B. Mobasher | J. Stott | D. Sobral | P. Best | J. Matthee | B. Darvish | S. Hemmati | H. Nayyeri | A. A. Khostovan | A. Khostovan | D. Sobral