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

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Berta,  S.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Bongiovanni, Á., Oteo, I., Cepa, J., Pérez García, A. M., Sánchez-Portal, M., Ederoclite, A., Aguerri, J. A. L., Alfaro, E. J., Altieri, B., Andreani, P., Aparicio-Villegas, M. T., Aussel, H., Benítez, N., Berta, S., Broadhurst, T., Cabrera-Caño, J., Castander, F. J., Cava, A., Cerviño, M., Chulani, H., Cimatti, A., Cristóbal-Hornillos, D., Daddi, E., Dominguez, H., Elbaz, D., Fernández-Soto, A., Förster Schreiber, N., Genzel, R., Gómez, M. F., González Delgado, R. M., Grazian, A., Gruppioni, C., Herreros, J. M., Iglesias Groth, S., Infante, L., Lutz, D., Magnelli, B., Magdis, G., Maiolino, R., Márquez, I., Martínez, V. J., Masegosa, J., Moles, M., Molino, A., Nordon, R., del Olmo, A., Perea, J., Poglitsch, A., Popesso, P., Pozzi, F., Prada, F., Quintana, J. M., Riguccini, L., Rodighiero, G., Saintonge, A., Sánchez, S. F., Santini, P., Shao, L., Sturm, E., Tacconi, L., & Valtchanov, I. (2010). Herschel FIR counterparts of selected Lyα emitters at z ~ 2.2 - Fast evolution since z ~ 3 or missed obscured AGNs? Astronomy & Astrophysics, 519:, pp. 1-9. doi:10.1051/0004-6361/201014719.


引用: https://hdl.handle.net/11858/00-001M-0000-0012-E05E-6
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