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Herschel FIR counterparts of selected Lyα emitters at z ∼2.2: Fast evolution since z∼3 or missed obscured AGNs? by Bongiovanni, A, Oteo, I, Cepa, J, Pérez García, A, Sánchez-Portal, M, Ederoclite, A, Aguerri, J, Alfaro, E, Altieri, B, Andreani, P, Aparicio-Villegas, M, Aussel, H, Benítez, N, Berta, S, Broadhurst, T, Cabrera-Caño, J, Castander, F, Cava, A, Cerviño, M, Chulani, H, Cimatti, A, Cristóbal-Hornillos, D, Daddi, E, Dominguez, H, Elbaz, D
Published 2010Journal article -
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Herschel FIR counterparts of selected Ly alpha emitters at z similar to 2.2 Fast evolution since z similar to 3 or missed obscured AGNs? by Bongiovanni, A, Oteo, I, Cepa, J, Perez Garcia, A, Sanchez-Portal, M, Ederoclite, A, Aguerri, J, Alfaro, E, Altieri, B, Andreani, P, Aparicio-Villegas, M, Aussel, H, Benitez, N, Berta, S, Broadhurst, T, Cabrera-Cano, J, Castander, F, Cava, A, Cervino, M, Chulani, H, Cimatti, A, Cristobal-Hornillos, D, Daddi, E, Dominguez, H, Elbaz, D
Published 2010Journal article