CEERS Key Paper. III. The Diversity of Galaxy Structure and Morphology at z=3-9 with JWST

被引:79
|
作者
Kartaltepe, Jeyhan S. [1 ]
Rose, Caitlin [1 ]
Vanderhoof, Brittany N. [1 ]
McGrath, Elizabeth J. [2 ]
Costantin, Luca [3 ]
Cox, Isabella G. [1 ]
Yung, L. Y. Aaron [4 ]
Kocevski, Dale D. [2 ]
Wuyts, Stijn [5 ]
Ferguson, Henry C. [6 ]
Bagley, Micaela B. [7 ]
Finkelstein, Steven L. [7 ]
Amorin, Ricardo O. [8 ,9 ]
Andrews, Brett H. [10 ,11 ]
Haro, Pablo Arrabal [12 ]
Backhaus, Bren E. [13 ]
Behroozi, Peter [14 ,15 ,16 ]
Bisigello, Laura [17 ,18 ]
Calabro, Antonello [19 ]
Casey, Caitlin M. [7 ]
Coogan, Rosemary T. [20 ]
Cooper, M. C. [21 ]
Croton, Darren [22 ,23 ]
de la Vega, Alexander [24 ]
Dickinson, Mark [38 ]
Fontana, Adriano [19 ]
Franco, Maximilien [7 ]
Grazian, Andrea [18 ]
Grogin, Norman A. [6 ]
Hathi, Nimish P. [6 ]
Holwerda, Benne W. [25 ]
Huertas-Company, Marc [26 ,27 ,28 ]
Iyer, Kartheik G. [29 ]
Jogee, Shardha [7 ]
Jung, Intae [6 ]
Kewley, Lisa J. [30 ]
Kirkpatrick, Allison [31 ]
Koekemoer, Anton M. [6 ]
Liu, James [1 ]
Lotz, Jennifer M. [32 ]
Lucas, Ray A. [6 ]
Newman, Jeffrey A. [33 ,34 ]
Pacifici, Camilla [6 ]
Pandya, Viraj [35 ]
Papovich, Casey [36 ,37 ]
Pentericci, Laura [19 ]
Perez-Gonzalez, Pablo G. [3 ]
Petersen, Jayse [1 ]
Pirzkal, Nor [6 ]
Rafelski, Marc [6 ]
机构
[1] Rochester Inst Technol, Sch Phys & Astron, Lab Multiwavelength Astrophys, 84 Lomb Mem Dr, Rochester, NY 14623 USA
[2] Colby Coll, Dept Phys & Astron, Waterville, ME 04901 USA
[3] CSIC INTA, Ctr Astrobiol CAB, Ctra Ajalvir Km 4, E-28850 Madrid, Spain
[4] NASA, Astrophys Sci Div, Goddard Space Flight Ctr, 8800 Greenbelt Rd, Greenbelt, MD 20771 USA
[5] Univ Bath, Dept Phys, Bath BA2 7AY, Avon, England
[6] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA
[7] Univ Texas Austin, Dept Astron, Austin, TX USA
[8] Univ La Serena, Inst Invest Multidisciplinar Ciencia & Tecnol, Raul Bitran 1305, La Serena 2204000, Chile
[9] Univ La Serena, Dept Astron, Ave Juan Cisternas 1200 Norte, La Serena 1720236, Chile
[10] Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA
[11] Univ Pittsburgh, Pittsburgh Particle Phys Astrophys & Cosmol Ctr P, Pittsburgh, PA 15260 USA
[12] NSFs Natl Opt Infrared Astron Res Lab, 950 North Cherry Ave, Tucson, AZ 85719 USA
[13] Univ Connecticut, Dept Phys, 196 Auditorium Rd,Unit 3046, Storrs, CT 06269 USA
[14] Univ Arizona, Dept Astron, Tucson, AZ 85721 USA
[15] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
[16] Natl Astron Observ Japan, Div Sci, 2 21-1 Osawa, Mitaka, Tokyo 1818588, Japan
[17] Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy
[18] INAF Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35122 Padua, Italy
[19] INAF Osservatorio Astron Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Italy
[20] Univ Paris Cite, Univ Paris Saclay, Sorbonne Paris Cite, CEA,IRFU,DAp,AIM,CNRS, F-91191 Gif Sur Yvette, France
[21] Univ Calif Irvine, Dept Phys & Astron, 4129 Reines Hall, Irvine, CA 92697 USA
[22] Swinburne Univ Technol, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia
[23] ARC Ctr Excellence All Sky Astrophys 3 Dimens AST, Melbourne, Vic, Australia
[24] Univ Calif Riverside, Dept Phys & Astron, Riverside, CA 92521 USA
[25] Univ Louisville, Phys & Astron Dept, Louisville, KY 40292 USA
[26] Inst Astrofis Canarias, San Cristobal la Laguna, Tenerife, Spain
[27] Univ La Laguna, San Cristobal la Laguna, Tenerife, Spain
[28] Univ Paris Cite, Observ Paris, PSL, LERMA, Paris, France
[29] Univ Toronto, Dunlap Inst Astron & Astrophys, Toronto, ON M5S 3H4, Canada
[30] Harvard & Smithsonian, Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
[31] Univ Kansas, Dept Phys & Astron, Lawrence, KS 66045 USA
[32] NSFs Natl Opt Infrared Astron Res Lab, Gemini Observ, 950 North Cherry Ave, Tucson, AZ 85719 USA
[33] Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA
[34] Univ Pittsburgh, PITT PACC, Pittsburgh, PA 15260 USA
[35] Columbia Univ, Columbia Astrophys Lab, 550 West 120th St, New York, NY 10027 USA
[36] Texas A&M Univ, Dept Phys & Astron, College Stn, TX 77843 USA
[37] Texas A&M Univ, George P & Cynthia Woods Mitchell Inst Fundamenta, College Stn, TX 77843 USA
[38] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA
[39] Flatiron Inst, Ctr Comp Astrophys, 162 5th Ave, New York, NY 10010 USA
[40] Univ Warwick, Dept Phys, Coventry CV4 7AL, W Midlands, England
[41] Univ Cambridge, Kavli Inst Cosmol, Madingley Rd, Cambridge CB3 0HA, England
[42] Univ Cambridge, Cavendish Lab, 19 JJ Thomson Ave, Cambridge CB3 0HE, England
[43] Univ Sussex, Astron Ctr, Brighton BN1 9QH, E Sussex, England
[44] Univ Malta, Inst Space Sci & Astron, MSD-2080 Msida, Malta
[45] Univ Groningen, Kapteyn Astron Inst, POB 800, NL-9700 AV Groningen, Netherlands
[46] SRON Netherlands Inst Space Res, POB 800, NL-9700 AV Groningen, Netherlands
[47] Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan
关键词
STAR-FORMING GALAXIES; ILLUSTRISTNG SIMULATIONS; DEEP-FIELD; MULTIWAVELENGTH MEASUREMENT; SEMIANALYTIC FORECASTS; LIGHT-CONES; EVOLUTION; CANDELS; REDSHIFT; STELLAR;
D O I
10.3847/2041-8213/acad01
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a comprehensive analysis of the evolution of the morphological and structural properties of a large sample of galaxies at z = 3-9 using early James Webb Space Telescope (JWST) CEERS NIRCam observations. Our sample consists of 850 galaxies at z > 3 detected in both Hubble Space Telescope (HST)/WFC3 and CEERS JWST/NIRCam images, enabling a comparison of HST and JWST morphologies. We conduct a set of visual classifications, with each galaxy in the sample classified three times. We also measure quantitative morphologies across all NIRCam filters. We find that galaxies at z > 3 have a wide diversity of morphologies. Galaxies with disks make up 60% of galaxies at z = 3, and this fraction drops to similar to 30% at z = 6-9, while galaxies with spheroids make up similar to 30%-40% across the redshift range, and pure spheroids with no evidence for disks or irregular features make up similar to 20%. The fraction of galaxies with irregular features is roughly constant at all redshifts (similar to 40%-50%), while those that are purely irregular increases from similar to 12% to similar to 20% at z > 4.5. We note that these are apparent fractions, as many observational effects impact the visibility of morphological features at high redshift. On average, Spheroid-only galaxies have a higher Sersic index, smaller size, and higher axis ratio than disk or irregular galaxies. Across all redshifts, smaller spheroid and disk galaxies tend to be rounder. Overall, these trends suggest that galaxies with established disks and spheroids exist across the full redshift range of this study, and further work with large samples at higher redshift is needed to quantify when these features first formed.
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页数:17
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