Crimson Behemoth: A massive clumpy structure hosting a dusty AGN at z=4.91

Publications of the Astronomical Society of Japan, Dec 2024

The current paradigm for the co-evolution of galaxies and their supermassive black holes postulates that dust-obscured active galactic nuclei (AGNs) represent a transitional phase towards a more luminous and unobscured state. However, our understanding of dusty AGNs and their host galaxies at early cosmic times is inadequate due to observational limitations. Here, we present JWST observations of CID-931, an X-ray-detected AGN at a spectroscopic redshift of |$z_{\rm spec}=4.91$|⁠. Multiband NIRCam imaging from the COSMOS-Web program reveals an unresolved red core, similar to JWST-discovered dusty AGNs. Strikingly, the red core is surrounded by at least eight massive star-forming clumps spread over |${1{^{\prime \prime}_{.}}6} \approx 10\,\,{\rm kpc}$|⁠, each of which has a stellar mass of |$10^9$|–|$10^{10}\, M_{\odot }$| and a radius of |$\sim$|0.1–1 kpc. The whole system amounts to |$10^{11}\, M_{\odot }$| in stellar mass, higher than typical star-forming galaxies at the same epoch. In this system, gas inflows and/or complex merger events may trigger clump formation and AGN activity, thus leading to the rapid formation of a massive galaxy hosting a supermassive black hole. Future follow-up observations will provide new insights into the evolution of the galaxy–black hole relationship during such transitional phases in the early universe.

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Crimson Behemoth: A massive clumpy structure hosting a dusty AGN at z=4.91

Publications of the Astronomical Society of Japan, 2024, 76(6), 1323–1335 https://doi.org/10.1093/pasj/psae091 Advance access publication date: 2024 November 4 Crimson Behemoth: A massive clumpy structure hosting a dusty AGN at z = 4.91 1 Department of Astronomy, Graduate School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, The University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583, Japan 3 Center for Data-Driven Discovery, Kavli IPMU (WPI), UTIAS, The University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583, Japan 4 Center for Astrophysical Sciences, Department of Physics and Astronomy, Johns Hopkins University, 3400 N. Charles Street, Baltimore, MD 21218, USA 5 Department of Physics, The University of Tokyo, 7-3-1 Hongo, Bunkyo, Tokyo 113-0033, Japan 6 Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, China 7 Research Center for the Early Universe, Graduate School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan 8 Center for Frontier Science, Chiba University, 1-33 Yayoi-cho, Inage-ku, Chiba 263-8522, Japan 9 Department of Astronomy, The University of Texas at Austin, 2515 Speedway Boulevard Stop C1400, Austin, TX 78712, USA 10 Cosmic Dawn Center (DAWN), Niels Bohr Building, Radmandsgade 62–64, DK-2200 Copenhagen N, Denmark 11 School of Physics and Technology, Wuhan University, Wuhan 430072, China 12 Caltech/IPAC, 1200 E. California Blvd., Pasadena, CA 91125, USA 13 European Southern Observatory, Karl-Schwarzschild-Str. 2, D-85748 Garching, Germany 14 DTU Space, Technical University of Denmark, Building 327, Elektrovej, DK-2800 Kgs. Lyngby, Denmark 15 Center for Computational Astrophysics, Flatiron Institute, 162 Fifth Avenue, New York, NY 10010, USA 16 Kapteyn Astronomical Institute, University of Groningen, NL-9700 AV Groningen, The Netherlands 17 Departamento de Fisica Teorica, Modulo 8, Facultad de Ciencias, Universidad Autonoma de Madrid, E-28049 Madrid, Spain 18 CIAFF, Facultad de Ciencias, Universidad Autonoma de Madrid, E-28049 Madrid, Spain 19 Department of Physics, University of Miami, 1320 Campo Sano Drive, Coral Gables, FL 33124, USA 20 Department of Astronomy, School of Physics, Peking University, 209 Chengfu Road, Haidian District, Beijing 100871, China 21 Technical University of Munich, TUM School of Natural Sciences, Department of Physics, James-Franck-Str. 1, D-85748 Garching, Germany 22 Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, D-85748 Garching, Germany 23 NASA-Goddard Space Flight Center, Code 662, Greenbelt, MD 20771, USA 24 Laboratory for Multiwavelength Astrophysics, School of Physics and Astronomy, Rochester Institute of Technology, 84 Lomb Memorial Drive, Rochester, NY 14623, USA 25 Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA 26 Institut d’Astrophysique de Paris, UMR 7095, CNRS, and Sorbonne Université, 98 bis boulevard Arago, F-75014 Paris, France 27 Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91001, USA 28 Department of Astronomy and Astrophysics, University of California, Santa Cruz, 1156 High Street, Santa Cruz, CA 95064, USA 29 Purple Mountain Observatory, Chinese Academy of Sciences, 10 Yuanhua Road, Nanjing 210023, China 30 The Observatories of the Carnegie Institution for Science, 813 Santa Barbara St., Pasadena, CA 91101, USA 31 Department of Computer Science, Aalto University, PO Box 15400, FI-00076 Espoo, Finland 32 Department of Physics, Faculty of Science, University of Helsinki, FI-00014 Helsinki, Finland 33 Institute for Physics, Laboratory for Galaxy Evolution and Spectral Modelling, Ecole Polytechnique Federale de Lausanne, Observatoire de Sauverny, Chemin Pegasi 51, CH-1290 Versoix, Switzerland 2 Received: 2024 August 22; Accepted: 2024 October 2 © The Author(s) 2024. Published by Oxford University Press on behalf of the Astronomical Society of Japan. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited. Takumi S. TANAKA ,1 ,2 ,3 ,∗ John D. SILVERMAN ,1 ,2 ,3 ,4 Yurina NAKAZATO ,5 Masafusa ONOUE ,2 ,6 Kazuhiro SHIMASAKU ,1 ,7 Yoshinobu FUDAMOTO ,8 Seiji FUJIMOTO ,9 ,10 Xuheng DING ,11 Andreas L. FAISST ,12 Francesco VALENTINO ,10 ,13 Shuowen JIN ,10 ,14 Christopher C. HAYWARD ,15 Vasily KOKOREV ,9 ,16 Daniel CEVERINO ,17 ,18 Boris S. KALITA ,2 ,3 ,6 Caitlin M. CASEY ,9 ,10 Zhaoxuan LIU ,1 ,2 ,3 Aidan KAMINSKY ,19 Qinyue FEI ,20 Irham T. ANDIKA ,21 ,22 Erini LAMBRIDES ,23 Hollis B. AKINS ,9 Jeyhan S. KARTALTEPE ,24 Anton M. KOEKEMOER ,25 Henry Joy MCCRACKEN ,26 Jason RHODES ,27 Brant E. ROBERTSON ,28 Maximilien FRANCO ,9 Daizhong LIU ,29 Nima CHARTAB ,30 Steven GILLMAN ,10 ,14 Ghassem GOZALIASL ,31 ,32 Michaela HIRSCHMANN ,33 ,34 Marc HUERTAS-COMPANY ,35 ,36 ,37 ,38 ,39 Richard MASSEY ,40 Namrata ROY ,4 Zahra SATTARI ,30 ,41 Marko SHUNTOV ,26 Joseph STERLING ,19 Sune TOFT ,10 ,42 Benny TRAKHTENBROT ,43 Naoki YOSHIDA ,2 ,5 ,7 and Jorge A. ZAVALA 44 1324 Publications of the Astronomical Society of Japan (2024), Vol. 76, No. 6 34 INAF, Osservatorio Astronomico di Trieste, Via Tiepolo 11, I-34131 Trieste, Italy Instituto de AstrofÃsica de Canarias (IAC), E-38205 La Laguna, Spain 36 Observatoire de Paris, LERMA, PSL University, 61 avenue de l’Observatoire, F-75014 Paris, France 37 Université Paris-Cité, 5 rue Thomas Mann, F-75014 Paris, France 38 Universidad de La Laguna, Avda. Astrofísico Fco. Sanchez, E-38205 La Laguna, Tenerife, Spain 39 Center for Computational Astrophysics, Flatiron Institute, 162 5th Avenue, New York, NY 10010, USA 40 Institute for Computational Cosmology, Department of Physics, Durham University, South Road, Durham DH1 3LE, UK 41 Department of Physics and Astronomy, University of California, Riverside, 900 University Ave., Riverside, CA 92521, USA 42 Niels Bohr Institute, University of Copenhagen, Jagtvej 128, DK-2200 Copenhagen N, Denmark 43 School of Physics and Astronomy, Tel Aviv University, Tel Aviv 69978, Israel 44 National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan 35 ∗ E-mail: The current paradigm for the co-evolution of galaxies and their supermassive black holes postulates that dust-obscured active galactic nuclei (AGNs) represent a transitional phase towards a more luminous and unobscured state. However, our understanding of dusty AGNs and their host galaxies at early cosmic times is inadequate due to observational limitations. Here, we present JWST observations of CID-931, an X-raydetected AGN at a spectroscopic redshift of zspec = 4.91. Multiband NIRCam imaging from the (...truncated)


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Tanaka, Takumi S, Silverman, John D, Nakazato, Yurina, Onoue, Masafusa, Shimasaku, Kazuhiro, Fudamoto, Yoshinobu, Fujimoto, Seiji, Ding, Xuheng, Faisst, Andreas L, Valentino, Francesco, Jin, Shuowen, Hayward, Christopher C, Kokorev, Vasily, Ceverino, Daniel, Kalita, Boris S, Casey, Caitlin M, Liu, Zhaoxuan, Kaminsky, Aidan, Fei, Qinyue, Andika, Irham T, Lambrides, Erini, Akins, Hollis B, Kartaltepe, Jeyhan S, Koekemoer, Anton M, McCracken, Henry Joy, Rhodes, Jason, Robertson, Brant E, Franco, Maximilien, Liu, Daizhong, Chartab, Nima, Gillman, Steven, Gozaliasl, Ghassem, Hirschmann, Michaela, Huertas-Company, Marc, Massey, Richard, Roy, Namrata, Sattari, Zahra, Shuntov, Marko, Sterling, Joseph, Toft, Sune, Trakhtenbrot, Benny, Yoshida, Naoki, Zavala, Jorge A. Crimson Behemoth: A massive clumpy structure hosting a dusty AGN at z=4.91, Publications of the Astronomical Society of Japan, 2024, pp. 1323-1335, Volume 76, Issue 6, DOI: 10.1093/pasj/psae091