CEERS Key Paper. II. A First Look at the Resolved Host Properties of AGN at 3 < z < 5 with JWST

被引：27

作者：

Kocevski, Dale D. ^{[1
]}

Barro, Guillermo ^{[2
]}

McGrath, Elizabeth J. ^{[1
]}

Finkelstein., Steven L. ^{[3
]}

Bagley., Micaela B. ^{[3
]}

Ferguson, Henry C. ^{[4
]}

Jogee, Shardha ^{[3
]}

Yang, Guang ^{[5
,6
]}

Dickinson, Mark ^{[7
]}

Hathi, Nimish P. ^{[4
]}

Backhaus, Bren E. ^{[8
]}

Bell, Eric F. ^{[9
]}

Bisigello, Laura ^{[10
,11
]}

Buat, Veronique ^{[12
]}

Burgarella, Denis ^{[12
]}

Casey, Caitlin M. ^{[3
]}

Cleri, Nikko J. ^{[13
,14
]}

Cooper, M. C. ^{[15
]}

Costantin, Luca ^{[16
]}

Croton, Darren ^{[17
,18
]}

Daddi, Emanuele ^{[19
]}

Fontana, Adriano ^{[20
]}

Fujimoto, Seiji ^{[21
,22
,23
]}

Gardner, Jonathan P. ^{[24
]}

Gawiser, Eric ^{[25
]}

Giavalisco, Mauro ^{[26
]}

Grazian, Andrea ^{[11
]}

Grogin, Norman A. ^{[4
]}

Guo, Yuchen ^{[3
]}

Haro, Pablo Arrabal ^{[7
]}

Hirschmann, Michaela ^{[27
]}

Holwerda, Benne W. ^{[28
]}

Huertas-Company, Marc ^{[29
,30
,31
]}

Hutchison, Taylor A. ^{[13
,14
,32
]}

Iyer, Kartheik G. ^{[33
]}

Jones, Brenda ^{[34
]}

Juneau, Stephanie ^{[35
]}

Kartaltepe, Jeyhan S. ^{[36
]}

Kewley, Lisa J. ^{[37
]}

Kirkpatrick, Allison ^{[38
]}

Koekemoer, Anton M. ^{[39
]}

Kurczynski, Peter ^{[40
]}

Le Bail, Aurelien ^{[19
]}

Long, Arianna S. ^{[21
]}

Lotz, Jennifer M. ^{[41
]}

Lucas, Ray A. ^{[39
]}

Papovich, Casey ^{[13
,14
]}

Pentericci, Laura ^{[20
]}

Perez-Gonzalez, Pablo G. ^{[42
]}

Pirzkal, Nor ^{[43
]}

机构：

[1] Colby Coll, Dept Phys & Astron, Waterville, ME 04901 USA

[2] Univ Pacific, Dept Phys, Stockton, CA 90340 USA

[3] Univ Texas Austin, Dept Astron, RLM 15308, Austin, TX 78712 USA

[4] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA

[5] Univ Groningen, Kapteyn Astron Inst, POB 800, NL-9700 AV Groningen, Netherlands

[6] SRON Netherlands Inst Space Res, Postbus 800, NL-9700 AV Groningen, Netherlands

[7] NSF, Natl Opt Infrared Astron Res Lab, 950 North Cherry Ave, Tucson, AZ 85719 USA

[8] Univ Connecticut, Dept Phys, 196 Auditorium Rd,Unit 3046, Storrs, CT 06269 USA

[9] Univ Michigan, Dept Astron, 1085 South Univ Ave, Ann Arbor, MI 48109 USA

[10] Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy

[11] Osserv Astron Padova, INAF, Vicolo Osservatorio 5, I-35122 Padua, Italy

[12] Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France

[13] Texas A&M Univ, Dept Phys & Astron, College Stn, TX 77843 USA

[14] Texas A&M Univ, George P & Cynthia Woods Mitchell Inst Fundamenta, College Stn, TX 77843 USA

[15] Univ Calif Irvine, Dept Phys & Astron, 4129 Reines Hall, Irvine, CA 92697 USA

[16] Ctr Astrobiol CSIC INTA, Ctra Ajalvir Km 4, E-28850 Madrid, Spain

[17] Swinburne Univ Technol, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia

[18] ARC Ctr Excellence All Sky Astrophys 3 Dimens AST, Stromlo, ACT, Australia

[19] Univ Paris Cite, Univ Paris Saclay, CEA, CNRS,AIM, F-91191 Gif Sur Yvette, France

[20] Osserv Astron Roma, INAF, Via Frascati 33, I-00078 Monte Porzio Catone, Italy

[21] Univ Texas Austin, Dept Astron, RLM 15308, Austin, TX 78712 USA

[22] Cosm Dawn Ctr DAWN, Jagtvej 128, DK-2200 Copenhagen N, Denmark

[23] Univ Copenhagen, Niels Bohr Inst, Lyngbyvej 2, DK-2100 Copenhagen O, Denmark

[24] Goddard Space Flight Ctr, Astrophys Sci Div, Code 665, Greenbelt, MD 20771 USA

[25] Rutgers State Univ, Dept Phys & Astron, Piscataway, NJ 08854 USA

[26] Univ Massachusetts, 710 North Pleasant St, Amherst, MA 01003 USA

[27] EPFL, Lab Galaxy Evolut, Inst Phys, Observ Sauverny, CH-1290 Versoix, Switzerland

[28] Univ Louisville, Dept Phys & Astron, Louisville, KY 40292 USA

[29] Inst Astrofis Canarias, Tenerife, Spain

[30] Univ La Laguna, Tenerife, Spain

[31] Univ Paris Cite, PSL, LERMA, Observ Paris, Paris, France

[32] NASA, Goddard Space Flight Ctr, Astrophys Sci Div, 8800 Greenbelt Rd, Greenbelt, MD 20771 USA

[33] Univ Toronto, Dunlap Inst Astron & Astrophys, Toronto, ON M5S 3H4, Canada

[34] Univ Maine, Dept Phys & Astron, Orono, ME 04469 USA

[35] NSFs NOIRLab, 950 North Cherry Ave, Tucson, AZ 85719 USA

[36] Rochester Inst Technol, Sch Phys & Astron, Lab Multiwavelength Astrophys, 84 Lomb Mem Dr, Rochester, NY 14623 USA

[37] Harvard & Smithsonian, Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA

[38] Univ Kansas, Dept Phys & Astron, Lawrence, KS 66045 USA

[39] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA

[40] NASA, Goddard Space Flight Ctr, Observat Cosmol Lab, Code 665, Greenbelt, MD 20771 USA

[41] NSF, Natl Opt Infrared Astron Res Lab, Gemini Observ, 950 North Cherry Ave, Tucson, AZ 85719 USA

[42] CSIC, INTA, Ctr Astrobiol CAB, Ctra Ajalvir Km 4, E-28850 Madrid, Spain

[43] ESA AURA Space Telescope Sci Inst, Baltimore, MD USA

[44] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA

[45] Flatiron Inst, Ctr Computat Astrophys, 162 5th Ave, New York, NY 10010 USA

[46] Univ Cambridge, Kavli Inst Cosmol, Madingley Rd, Cambridge CB3 0HA, England

[47] Univ Cambridge, Cavendish Lab, 19 JJ Thomson Ave, Cambridge CB3 0HE, England

[48] Univ Sussex, Ctr Astron, Brighton BN1 9QH, E Sussex, England

[49] Univ Malta, Inst Space Sci & Astron, MSD-2080 Msida, Malta

[50] Univ Bath, Dept Phys, Bath BA2 7AY, Avon, England

来源：

ASTROPHYSICAL JOURNAL LETTERS | 2023年 / 946卷 / 01期

关键词：

SUPERMASSIVE BLACK-HOLES; SIMILAR-TO; 2; ACTIVE GALACTIC NUCLEI; STAR-FORMATION RATE; STELLAR POPULATION SYNTHESIS; COLOR-MAGNITUDE RELATION; DEBLENDED DUST EMISSION; DIGITAL SKY SURVEY; MASSIVE GALAXIES; QUIESCENT GALAXIES;

D O I：

10.3847/2041-8213/acad00

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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.

引用

页数：14

共 6 条

[1] CEERS Key Paper. I. An Early Look into the First 500 Myr of Galaxy Formation with JWST
Finkelstein, Steven L.
Bagley, Micaela B.
Ferguson, Henry C.
Wilkins, Stephen M.
Kartaltepe, Jeyhan S.
Papovich, Casey
Yung, L. Y. Aaron
Haro, Pablo Arrabal
Behroozi, Peter
Dickinson, Mark
Kocevski, Dale D.
Koekemoer, Anton M.
Larson, Rebecca L.
Le Bail, Aurelien
Morales, Alexa M.
Perez-Gonzalez, Pablo G.
Burgarella, Denis
Dave, Romeel
Hirschmann, Michaela
Somerville, Rachel S.
Wuyts, Stijn
Bromm, Volker
Casey, Caitlin M.
Fontana, Adriano
Fujimoto, Seiji
Gardner, Jonathan P.
Giavalisco, Mauro
Grazian, Andrea
Grogin, Norman A.
Hathi, Nimish P.
Hutchison, Taylor A.
Jha, Saurabh W.
Jogee, Shardha
Kewley, Lisa J.
Kirkpatrick, Allison
Long, Arianna S.
Lotz, Jennifer M.
Pentericci, Laura
Pierel, Justin D. R.
Pirzkal, Nor
Ravindranath, Swara
Ryan, Russell E.
Trump, Jonathan R.
Yang, Guang
Bhatawdekar, Rachana
Bisigello, Laura
Buat, Veronique
Calabro, Antonello
Castellano, Marco
Cleri, Nikko J.
ASTROPHYSICAL JOURNAL LETTERS, 2023, 946 (01)
[2] CEERS Key Paper. III. The Diversity of Galaxy Structure and Morphology at z=3-9 with JWST
Kartaltepe, Jeyhan S.
Rose, Caitlin
Vanderhoof, Brittany N.
McGrath, Elizabeth J.
Costantin, Luca
Cox, Isabella G.
Yung, L. Y. Aaron
Kocevski, Dale D.
Wuyts, Stijn
Ferguson, Henry C.
Bagley, Micaela B.
Finkelstein, Steven L.
Amorin, Ricardo O.
Andrews, Brett H.
Haro, Pablo Arrabal
Backhaus, Bren E.
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Coogan, Rosemary T.
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Dickinson, Mark
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Grogin, Norman A.
Hathi, Nimish P.
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Jogee, Shardha
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Liu, James
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ASTROPHYSICAL JOURNAL LETTERS, 2023, 946 (01)
[3] CEERS Key Paper. VI. JWST/MIRI Uncovers a Large Population of Obscured AGN at High Redshifts
Yang, G.
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Papovich, C.
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ASTROPHYSICAL JOURNAL LETTERS, 2023, 950 (01)
[4] A surprising abundance of massive quiescent galaxies at 3 < z < 5 in the first data from JWST CEERS
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Jewell, S. M.
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Wild, V.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2023, 520 (03) : 3974 - 3985
[5] SUPER: II. Spatially resolved ionised gas kinematics and scaling relations in z ∼ 2 AGN host galaxies
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ASTRONOMY & ASTROPHYSICS, 2020, 642 (642)
[6] EIGER. II. First Spectroscopic Characterization of the Young Stars and Ionized Gas Associated with Strong Hβ and [O iii] Line Emission in Galaxies at z=5-7 with JWST
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ASTROPHYSICAL JOURNAL, 2023, 950 (01):

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