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Aussel, H. Chulani, H. Dominguez, I. Marquez, I. Oteo, I. Valtchanov, J. A. L. Aguerri, J. Cabrera-Cano, J. Cepa, J. Masegosa, J. M. Herreros, J. M. Quintana, J. Perea, L. Infante, L. Riguccini, L. Shao, L. Tacconi, M. Cervino, M. F. Gomez, M. Moles, M. Sanchez-Portal, M. T. Aparicio-Villegas, N. Benitez, N. Forster Schreiber, P. Andreani, P. Popesso, P. Santini, R. Genzel, R. Maiolino, R. M. Gonzalez Delgado, R. Nordon, S. Berta, S. F. Sanchez, S. Iglesias-Groth, T. Broadhurst, V. J. Martinez","submitted_at":"2010-08-10T16:57:25Z","abstract_excerpt":"Ly-alpha 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. 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