Herschel FIR counterparts of selected Lyα emitters at z ∼2.2: Fast evolution since z∼3 or missed obscured AGNs?

Lyα emitters (LAEs) are seen everywhere in the redshift domain from local to z∼7. Far-infrared (FIR) counterparts of LAEs at different epochs could provide direct clues on dust content, extinction, and spectral energy distribution (SED) for these galaxies. We search for FIR counterparts of LAEs that...

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Bibliographic Details
Main Authors:	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
Format:	Journal article
Language:	English
Published:	2010

Herschel FIR counterparts of selected Lyα emitters at z ∼2.2: Fast evolution since z∼3 or missed obscured AGNs?

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