CEERS Key Paper. II. A First Look at the Resolved Host Properties of AGN at 3 < z < 5 with JWST
We report on the host properties of five X-ray-luminous active galactic nuclei (AGN) identified at 3 < z < 5 in the first epoch of imaging from the Cosmic Evolution Early Release Science Survey. Each galaxy has been imaged with the JWST Near-Infrared Camera, which provides rest-frame optical m...
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| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2023-01-01
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| Series: | The Astrophysical Journal Letters |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/2041-8213/acad00 |
| _version_ | 1797403163736670208 |
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| author | Dale D. Kocevski Guillermo Barro Elizabeth J. McGrath Steven L. Finkelstein Micaela B. Bagley Henry C. Ferguson Shardha Jogee Guang Yang Mark Dickinson Nimish P. Hathi Bren E. Backhaus Eric F. Bell Laura Bisigello Véronique Buat Denis Burgarella Caitlin M. Casey Nikko J. Cleri M. C. Cooper Luca Costantin Darren Croton Emanuele Daddi Adriano Fontana Seiji Fujimoto Jonathan P. Gardner Eric Gawiser Mauro Giavalisco Andrea Grazian Norman A. Grogin Yuchen Guo Pablo Arrabal Haro Michaela Hirschmann Benne W. Holwerda Marc Huertas-Company Taylor A. Hutchison Kartheik G. Iyer Brenda Jones Stéphanie Juneau Jeyhan S. Kartaltepe Lisa J. Kewley Allison Kirkpatrick Anton M. Koekemoer Peter Kurczynski Aurélien Le Bail Arianna S. Long Jennifer M. Lotz Ray A. Lucas Casey Papovich Laura Pentericci Pablo G. Pérez-González Nor Pirzkal Marc Rafelski Swara Ravindranath Rachel S. Somerville Amber N. Straughn Sandro Tacchella Jonathan R. Trump Stephen M. Wilkins Stijn Wuyts L. Y. Aaron Yung Jorge A. Zavala |
| author_facet | Dale D. Kocevski Guillermo Barro Elizabeth J. McGrath Steven L. Finkelstein Micaela B. Bagley Henry C. Ferguson Shardha Jogee Guang Yang Mark Dickinson Nimish P. Hathi Bren E. Backhaus Eric F. Bell Laura Bisigello Véronique Buat Denis Burgarella Caitlin M. Casey Nikko J. Cleri M. C. Cooper Luca Costantin Darren Croton Emanuele Daddi Adriano Fontana Seiji Fujimoto Jonathan P. Gardner Eric Gawiser Mauro Giavalisco Andrea Grazian Norman A. Grogin Yuchen Guo Pablo Arrabal Haro Michaela Hirschmann Benne W. Holwerda Marc Huertas-Company Taylor A. Hutchison Kartheik G. Iyer Brenda Jones Stéphanie Juneau Jeyhan S. Kartaltepe Lisa J. Kewley Allison Kirkpatrick Anton M. Koekemoer Peter Kurczynski Aurélien Le Bail Arianna S. Long Jennifer M. Lotz Ray A. Lucas Casey Papovich Laura Pentericci Pablo G. Pérez-González Nor Pirzkal Marc Rafelski Swara Ravindranath Rachel S. Somerville Amber N. Straughn Sandro Tacchella Jonathan R. Trump Stephen M. Wilkins Stijn Wuyts L. Y. Aaron Yung Jorge A. Zavala |
| author_sort | Dale D. Kocevski |
| collection | DOAJ |
| description | We report on the host properties of five X-ray-luminous active galactic nuclei (AGN) identified at 3 < z < 5 in the first epoch of imaging from the Cosmic Evolution Early Release Science Survey. Each galaxy has been imaged with the JWST Near-Infrared Camera, which provides rest-frame optical morphologies at these redshifts. We also derive stellar masses and star formation rates for each host by fitting its spectral energy distribution using a combination of galaxy and AGN templates. We find that three of the AGN hosts have spheroidal morphologies, one is a bulge-dominated disk, and one is dominated by pointlike emission. None are found to show strong morphological disturbances that might indicate a recent interaction or merger event. When compared to a sample of mass-matched inactive galaxies, we find that the AGN hosts have morphologies that are less disturbed and more bulge-dominated. Notably, all four of the resolved hosts have rest-frame optical colors consistent with a quenched or poststarburst stellar population. The presence of AGN in passively evolving galaxies at z > 3 is significant because a rapid feedback mechanism is required in most semianalytic models and cosmological simulations to explain the growing population of massive quiescent galaxies observed at these redshifts. Our findings show that AGN can continue to inject energy into these systems after their star formation is curtailed, potentially heating their halos and preventing renewed star formation. Additional observations will be needed to determine what role this feedback may play in helping to quench these systems and/or maintain their quiescent state. |
| first_indexed | 2024-03-09T02:34:31Z |
| format | Article |
| id | doaj.art-757a628cbef246e58d7ed9319296d649 |
| institution | Directory Open Access Journal |
| issn | 2041-8205 |
| language | English |
| last_indexed | 2024-03-09T02:34:31Z |
| publishDate | 2023-01-01 |
| publisher | IOP Publishing |
| record_format | Article |
| series | The Astrophysical Journal Letters |
| spelling | doaj.art-757a628cbef246e58d7ed9319296d6492023-12-06T11:41:47ZengIOP PublishingThe Astrophysical Journal Letters2041-82052023-01-019461L1410.3847/2041-8213/acad00CEERS Key Paper. II. A First Look at the Resolved Host Properties of AGN at 3 < z < 5 with JWSTDale D. Kocevski0https://orcid.org/0000-0002-8360-3880Guillermo Barro1https://orcid.org/0000-0002-0786-7307Elizabeth J. McGrath2https://orcid.org/0000-0001-8688-2443Steven L. Finkelstein3https://orcid.org/0000-0001-8519-1130Micaela B. Bagley4https://orcid.org/0000-0002-9921-9218Henry C. Ferguson5https://orcid.org/0000-0001-7113-2738Shardha Jogee6https://orcid.org/0000-0002-1590-0568Guang Yang7https://orcid.org/0000-0001-8835-7722Mark Dickinson8https://orcid.org/0000-0001-5414-5131Nimish P. Hathi9https://orcid.org/0000-0001-6145-5090Bren E. Backhaus10https://orcid.org/0000-0001-8534-7502Eric F. Bell11https://orcid.org/0000-0002-5564-9873Laura Bisigello12https://orcid.org/0000-0003-0492-4924Véronique Buat13https://orcid.org/0000-0003-3441-903XDenis Burgarella14https://orcid.org/0000-0002-4193-2539Caitlin M. Casey15https://orcid.org/0000-0002-0930-6466Nikko J. Cleri16https://orcid.org/0000-0001-7151-009XM. C. Cooper17https://orcid.org/0000-0003-1371-6019Luca Costantin18https://orcid.org/0000-0001-6820-0015Darren Croton19https://orcid.org/0000-0002-5009-512XEmanuele Daddi20https://orcid.org/0000-0002-3331-9590Adriano Fontana21https://orcid.org/0000-0003-3820-2823Seiji Fujimoto22https://orcid.org/0000-0001-7201-5066Jonathan P. Gardner23https://orcid.org/0000-0003-2098-9568Eric Gawiser24https://orcid.org/0000-0003-1530-8713Mauro Giavalisco25https://orcid.org/0000-0002-7831-8751Andrea Grazian26https://orcid.org/0000-0002-5688-0663Norman A. Grogin27https://orcid.org/0000-0001-9440-8872Yuchen Guo28https://orcid.org/0000-0002-4162-6523Pablo Arrabal Haro29https://orcid.org/0000-0002-7959-8783Michaela Hirschmann30https://orcid.org/0000-0002-3301-3321Benne W. Holwerda31https://orcid.org/0000-0002-4884-6756Marc Huertas-Company32https://orcid.org/0000-0002-1416-8483Taylor A. Hutchison33https://orcid.org/0000-0001-6251-4988Kartheik G. Iyer34https://orcid.org/0000-0001-9298-3523Brenda Jones35Stéphanie Juneau36https://orcid.org/0000-0002-0000-2394Jeyhan S. Kartaltepe37https://orcid.org/0000-0001-9187-3605Lisa J. Kewley38https://orcid.org/0000-0001-8152-3943Allison Kirkpatrick39https://orcid.org/0000-0002-1306-1545Anton M. Koekemoer40https://orcid.org/0000-0002-6610-2048Peter Kurczynski41https://orcid.org/0000-0002-8816-5146Aurélien Le Bail42https://orcid.org/0000-0002-9466-2763Arianna S. Long43https://orcid.org/0000-0002-7530-8857Jennifer M. Lotz44https://orcid.org/0000-0003-3130-5643Ray A. Lucas45https://orcid.org/0000-0003-1581-7825Casey Papovich46https://orcid.org/0000-0001-7503-8482Laura Pentericci47https://orcid.org/0000-0001-8940-6768Pablo G. Pérez-González48https://orcid.org/0000-0003-4528-5639Nor Pirzkal49https://orcid.org/0000-0003-3382-5941Marc Rafelski50https://orcid.org/0000-0002-9946-4731Swara Ravindranath51https://orcid.org/0000-0002-5269-6527Rachel S. Somerville52https://orcid.org/0000-0002-6748-6821Amber N. Straughn53https://orcid.org/0000-0002-4772-7878Sandro Tacchella54https://orcid.org/0000-0002-8224-4505Jonathan R. Trump55https://orcid.org/0000-0002-1410-0470Stephen M. Wilkins56https://orcid.org/0000-0003-3903-6935Stijn Wuyts57https://orcid.org/0000-0003-3735-1931L. Y. Aaron Yung58https://orcid.org/0000-0003-3466-035XJorge A. Zavala59https://orcid.org/0000-0002-7051-1100Department of Physics and Astronomy , Colby College, Waterville, ME 04901, USA ; dale.kocevski@colby.eduDepartment of Physics, University of the Pacific , Stockton, CA 90340, USADepartment of Physics and Astronomy , Colby College, Waterville, ME 04901, USA ; dale.kocevski@colby.eduDepartment of Astronomy, The University of Texas at Austin , Austin, TX, USADepartment of Astronomy, The University of Texas at Austin , Austin, TX, USASpace Telescope Science Institute , Baltimore, MD, USADepartment of Astronomy, The University of Texas at Austin , Austin, TX, USAKapteyn Astronomical Institute, University of Groningen , P.O. Box 800, 9700 AV Groningen, The Netherlands; SRON Netherlands Institute for Space Research , Postbus 800, 9700 AV Groningen, The NetherlandsNSF’s National Optical-Infrared Astronomy Research Laboratory , 950 North Cherry Avenue, Tucson, AZ 85719, USASpace Telescope Science Institute , Baltimore, MD, USADepartment of Physics, University of Connecticut , 196 Auditorium Road, Unit 3046, Storrs, CT 06269, USADepartment of Astronomy, University of Michigan , 1085 South University Avenue, Ann Arbor, MI 48109-1107, USADipartimento di Fisica e Astronomia “G.Galilei,” Universitá di Padova , Via Marzolo 8, I-35131 Padova, Italy; INAF–Osservatorio Astronomico di Padova , Vicolo dell’Osservatorio 5, I-35122, Padova, ItalyAix Marseille Univ , CNRS, CNES, LAM Marseille, FranceAix Marseille Univ , CNRS, CNES, LAM Marseille, FranceDepartment of Astronomy, The University of Texas at Austin , Austin, TX, USADepartment of Physics and Astronomy, Texas A&M University , College Station, TX 77843-4242, USA; George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University , College Station, TX 77843-4242, USADepartment of Physics & Astronomy, University of California , Irvine, 4129 Reines Hall, Irvine, CA 92697, USACentro de Astrobiología (CSIC-INTA) , Ctra de Ajalvir km 4, Torrejón de Ardoz, E-28850, Madrid, SpainCentre for Astrophysics & Supercomputing, Swinburne University of Technology , Hawthorn, VIC 3122, Australia; ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D) , AustraliaUniversité Paris-Saclay , Université Paris Cité, CEA, CNRS, AIM, F-91191, Gif-sur-Yvette, FranceINAF–Osservatorio Astronomico di Roma , via di Frascati 33, I-00078 Monte Porzio Catone, ItalyDepartment of Astronomy, The University of Texas at Austin , Austin, TX 78712, USA; Cosmic Dawn Center (DAWN) , Jagtvej 128, DK-2200 Copenhagen N, Denmark; Niels Bohr Institute, University of Copenhagen , Lyngbyvej 2, DK-2100 Copenhagen Ø, DenmarkAstrophysics Science Division , Goddard Space Flight Center, Code 665, Greenbelt, MD 20771, USADepartment of Physics and Astronomy, Rutgers, the State University of New Jersey , Piscataway, NJ 08854, USAUniversity of Massachusetts Amherst , 710 North Pleasant Street, Amherst, MA 01003-9305, USAINAF–Osservatorio Astronomico di Padova , Vicolo dell’Osservatorio 5, I-35122, Padova, ItalySpace Telescope Science Institute , Baltimore, MD, USADepartment of Astronomy, The University of Texas at Austin , Austin, TX, USANSF’s National Optical-Infrared Astronomy Research Laboratory , 950 North Cherry Avenue, Tucson, AZ 85719, USAInstitute of Physics , Laboratory of Galaxy Evolution, Ecole Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, 1290 Versoix, SwitzerlandPhysics & Astronomy Department, University of Louisville , Louisville, KY 40292, USAInstituto de Astrofísica de Canarias , La Laguna, Tenerife, Spain; Universidad de la Laguna , La Laguna, Tenerife, Spain; Université Paris-Cité , LERMA—Observatoire de Paris, PSL, Paris, FranceDepartment of Physics and Astronomy, Texas A&M University , College Station, TX 77843-4242, USA; George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University , College Station, TX 77843-4242, USA; Astrophysics Science Division, NASA Goddard Space Flight Center , 8800 Greenbelt Road, Greenbelt, MD 20771, USADunlap Institute for Astronomy & Astrophysics, University of Toronto , Toronto, ON M5S 3H4, CanadaDepartment of Physics and Astronomy, University of Maine , Orono, ME 04469-5709, USANSF’s NOIRLab , 950 North Cherry Avenue, Tucson, AZ 85719, USALaboratory for Multiwavelength Astrophysics, School of Physics and Astronomy, Rochester Institute of Technology , 84 Lomb Memorial Drive, Rochester, NY 14623, USACenter for Astrophysics ∣ Harvard & Smithsonian , 60 Garden Street, Cambridge, MA 02138, USADepartment of Physics and Astronomy, University of Kansas , Lawrence, KS 66045, USASpace Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USAObservational Cosmology Laboratory (Code 665), NASA Goddard Space Flight Center , Greenbelt, MD 20771, USAUniversité Paris-Saclay , Université Paris Cité, CEA, CNRS, AIM, F-91191, Gif-sur-Yvette, FranceDepartment of Astronomy, The University of Texas at Austin , Austin, TX 78712, USAGemini Observatory/NSF’s National Optical-Infrared Astronomy Research Laboratory , 950 North Cherry Avenue, Tucson, AZ 85719, USASpace Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USADepartment of Physics and Astronomy, Texas A&M University , College Station, TX 77843-4242, USA; George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University , College Station, TX 77843-4242, USAINAF–Osservatorio Astronomico di Roma , via di Frascati 33, I-00078 Monte Porzio Catone, ItalyCentro de Astrobiología (CAB) , CSIC-INTA, Ctra. de Ajalvir km 4, Torrejón de Ardoz, E-28850, Madrid, SpainESA/AURA Space Telescope Science Institute , USASpace Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USA; Department of Physics and Astronomy, Johns Hopkins University , Baltimore, MD 21218, USASpace Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USACenter for Computational Astrophysics, Flatiron Institute , 162 5th Avenue, New York, NY 10010, USAAstrophysics Science Division, NASA Goddard Space Flight Center , 8800 Greenbelt Road, Greenbelt, MD 20771, USAKavli Institute for Cosmology, University of Cambridge , Madingley Road, Cambridge, CB3 0HA, UK; Cavendish Laboratory, University of Cambridge , 19 JJ Thomson Avenue, Cambridge, CB3 0HE, UKDepartment of Physics, University of Connecticut , 196 Auditorium Road, Unit 3046, Storrs, CT 06269, USAAstronomy Centre, University of Sussex , Falmer, Brighton BN1 9QH, UK; Institute of Space Sciences and Astronomy, University of Malta , Msida MSD 2080, MaltaDepartment of Physics, University of Bath , Claverton Down, Bath BA2 7AY, UKAstrophysics Science Division, NASA Goddard Space Flight Center , 8800 Greenbelt Road, Greenbelt, MD 20771, USANational Astronomical Observatory of Japan , 2-21-1 Osawa, Mitaka, Tokyo 181-8588, JapanWe report on the host properties of five X-ray-luminous active galactic nuclei (AGN) identified at 3 < z < 5 in the first epoch of imaging from the Cosmic Evolution Early Release Science Survey. Each galaxy has been imaged with the JWST Near-Infrared Camera, which provides rest-frame optical morphologies at these redshifts. We also derive stellar masses and star formation rates for each host by fitting its spectral energy distribution using a combination of galaxy and AGN templates. We find that three of the AGN hosts have spheroidal morphologies, one is a bulge-dominated disk, and one is dominated by pointlike emission. None are found to show strong morphological disturbances that might indicate a recent interaction or merger event. When compared to a sample of mass-matched inactive galaxies, we find that the AGN hosts have morphologies that are less disturbed and more bulge-dominated. Notably, all four of the resolved hosts have rest-frame optical colors consistent with a quenched or poststarburst stellar population. The presence of AGN in passively evolving galaxies at z > 3 is significant because a rapid feedback mechanism is required in most semianalytic models and cosmological simulations to explain the growing population of massive quiescent galaxies observed at these redshifts. Our findings show that AGN can continue to inject energy into these systems after their star formation is curtailed, potentially heating their halos and preventing renewed star formation. Additional observations will be needed to determine what role this feedback may play in helping to quench these systems and/or maintain their quiescent state.https://doi.org/10.3847/2041-8213/acad00AGN host galaxiesSupermassive black holes |
| spellingShingle | Dale D. Kocevski Guillermo Barro Elizabeth J. McGrath Steven L. Finkelstein Micaela B. Bagley Henry C. Ferguson Shardha Jogee Guang Yang Mark Dickinson Nimish P. Hathi Bren E. Backhaus Eric F. Bell Laura Bisigello Véronique Buat Denis Burgarella Caitlin M. Casey Nikko J. Cleri M. C. Cooper Luca Costantin Darren Croton Emanuele Daddi Adriano Fontana Seiji Fujimoto Jonathan P. Gardner Eric Gawiser Mauro Giavalisco Andrea Grazian Norman A. Grogin Yuchen Guo Pablo Arrabal Haro Michaela Hirschmann Benne W. Holwerda Marc Huertas-Company Taylor A. Hutchison Kartheik G. Iyer Brenda Jones Stéphanie Juneau Jeyhan S. Kartaltepe Lisa J. Kewley Allison Kirkpatrick Anton M. Koekemoer Peter Kurczynski Aurélien Le Bail Arianna S. Long Jennifer M. Lotz Ray A. Lucas Casey Papovich Laura Pentericci Pablo G. Pérez-González Nor Pirzkal Marc Rafelski Swara Ravindranath Rachel S. Somerville Amber N. Straughn Sandro Tacchella Jonathan R. Trump Stephen M. Wilkins Stijn Wuyts L. Y. Aaron Yung Jorge A. Zavala CEERS Key Paper. II. A First Look at the Resolved Host Properties of AGN at 3 < z < 5 with JWST The Astrophysical Journal Letters AGN host galaxies Supermassive black holes |
| title | CEERS Key Paper. II. A First Look at the Resolved Host Properties of AGN at 3 < z < 5 with JWST |
| title_full | CEERS Key Paper. II. A First Look at the Resolved Host Properties of AGN at 3 < z < 5 with JWST |
| title_fullStr | CEERS Key Paper. II. A First Look at the Resolved Host Properties of AGN at 3 < z < 5 with JWST |
| title_full_unstemmed | CEERS Key Paper. II. A First Look at the Resolved Host Properties of AGN at 3 < z < 5 with JWST |
| title_short | CEERS Key Paper. II. A First Look at the Resolved Host Properties of AGN at 3 < z < 5 with JWST |
| title_sort | ceers key paper ii a first look at the resolved host properties of agn at 3 z 5 with jwst |
| topic | AGN host galaxies Supermassive black holes |
| url | https://doi.org/10.3847/2041-8213/acad00 |
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