A hidden active galactic nucleus powering bright [O III] nebulae in a protocluster at <i>z</i> = 4.5 revealed by JWST
M. Solimano, L. Yan, N. M. Förster-Schreiber, M. Boquien(Universidad de Antofagasta), Ilse De Looze(Ghent University), M. Ginolfi, M. Relaño, J. González-López, S. Bovino, P. Ogle(Vassar College), F. Pozzi(University of Bologna), Dominik A. Riechers(Cornell University), Michael Romano(Max Planck Institute for Radio Astronomy), Roberto J. Assef, Nimish P. Hathi(Space Telescope Science Institute), D. Liu, Vicente Villanueva, Anton M. Koekemoer(Space Telescope Science Institute), Rodrigo Herrera-Camus, Gareth C. Jones(University of Oxford), Hanae Inami(Université Claude Bernard Lyon 1), L. Vallini, A. Ferrara, D. Vergani, Belén Alcalde Pampliega, Caitlin M. Casey, K. Telikova, M. Béthermin(Centre National de la Recherche Scientifique), C. Gruppioni, Nikolaus Sulzenauer, S. Fujimoto, Justin Spilker, L. Lee, S. Veilleux, R. L. Davies, Ana Posses, Elisabete da Cunha(Australian National University), Manuel Aravena, Juno Li, L. Guaita, Andreas L. Faisst(California Institute of Technology), T. Díaz-Santos, P. Cassata, E. Ibar(University of Valparaíso), Donald B. Fisher(Washington State University), J. Molina, Xuheng Ding, K. G. C. Vasan, Zhaoxuan Liu
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