Herschel ⋆ FIR counterparts of selected Lyα emitters at z2.2 Fast evolution since z3 or missed obscured AGNs?
Á. Bongiovanni, S. Iglesias Groth(Universidad de La Laguna), P. Andreani(European Southern Observatory), M. T. Aparicio-Villegas(Instituto de Astrofísica de Andalucía), A. Ederoclite(California Earthquake Authority), A. Grazian(Astronomical Observatory of Rome), D. Elbaz(Université Paris-Saclay), A. Cava(Universidad Complutense de Madrid), F. J. Castander(University of Chicago), J. Cepa(Instituto de Astrofísica de Canarias), B. Altieri(European Space Astronomy Centre), E. J. Alfaro(Instituto de Astrofísica de Andalucía), H. Chulani(Instituto de Astrofísica de Canarias), E. Daddi(Centre National de la Recherche Scientifique), S. Berta(Institut de Radioastronomie Millimétrique), C. Gruppioni(Osservatorio di Astrofisica e Scienza dello Spazio), A. Cimatti, I. Oteo(Cardiff University)
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