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 Hospital), 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(National Centre for Nuclear Research), 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(Waseda University), Hanae Inami(Université Claude Bernard Lyon 1), L. Vallini, A. Ferrara(Scuola Normale Superiore), D. Vergani, Belén Alcalde Pampliega, Caitlin M. Casey(University of California System), K. Telikova, M. Béthermin(Centre National de la Recherche Scientifique), C. Gruppioni, Nikolaus Sulzenauer, S. Fujimoto, Justin Spilker(The University of Texas at Austin), L. Lee, S. Veilleux, R. L. Davies, Ana Posses, Elisabete da Cunha(The University of Western Australia), 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(ARC Centre of Excellence for All-sky Astrophysics), J. Molina, Xuheng Ding, K. G. C. Vasan, Zhaoxuan Liu
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