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Bisigello, L. ; Caputi, K. I. ; Colina, L. ; Le Fèvre, O. ; Norgaard-Nielsen, H. U. ; Pérez González, Pablo Guillermo ; Van der Werf, P. ; Ilbert, O. ; Grogin, N. ; Koekemoer, A. | University Chicago Press | 2017-07Imaging with the James Webb Space Telescope (JWST) will allow observations of the bulk of distant galaxies at the epoch of reionization. The recovery of their properties, such as age, color excess E(B-V), specific star formation rate (sSFR), and[...]texto impreso
Álvarez Márquez, J. ; Burgarella, D. ; Buat, V. ; Ilbert, O. ; Pérez González, Pablo Guillermo | EDP Sciencies | 2019-10-09Aims. This work explores, from a statistical point of view, the rest-frame far-ultraviolet (FUV) to far-infrared (FIR) emission of a population of Lyman-break galaxies (LBGs) at z ? 3 that cannot be individually detected from current FIR observa[...]texto impreso
Bisigello, L. ; Caputi, K. I. ; Colina, L. ; Le Fèvre, O. ; Nørgaard-Nielsen, H. U. ; Pérez González, Pablo Guillermo ; Pye, J. ; Van der Werf, P. ; Ilbert, O. ; Grogin, N. ; Koekemoer, A. | IOP publishing ltd | 2016-12he determination of galaxy redshifts in the James Webb Space Telescope’s (JWST) blank-field surveys will mostly rely on photometric estimates, based on the data provided by JWST’s Near-Infrared Camera (NIRCam) at 0.6–5.0 ?m and Mid Infrared Inst[...]
