CEERS Key Paper. III. The Diversity of Galaxy Structure and Morphology at z = 3-9 with JWST
Date Issued
2023
Author(s)
Kartaltepe, Jeyhan S.
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Rose, Caitlin
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Vanderhoof, Brittany N.
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McGrath, Elizabeth J.
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COSTANTIN, LUCA
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Cox, Isabella G.
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Aaron Yung, L. Y.
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Kocevski, Dale D.
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Wuyts, Stijn
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Ferguson, Henry C.
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Bagley, Micaela B.
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Finkelstein, Steven L.
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Amorín, Ricardo O.
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Andrews, Brett H.
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Haro, Pablo Arrabal
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Backhaus, Bren E.
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Behroozi, Peter
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•
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Casey, Caitlin M.
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Coogan, Rosemary T.
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Cooper, M. C.
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Croton, Darren
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de la Vega, Alexander
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•
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Franco, Maximilien
•
•
Grogin, Norman A.
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Hathi, Nimish P.
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Holwerda, Benne W.
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Huertas-Company, Marc
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Iyer, Kartheik G.
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Jogee, Shardha
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Jung, Intae
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Kewley, Lisa J.
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Kirkpatrick, Allison
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Koekemoer, Anton M.
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Liu, James
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Lotz, Jennifer M.
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Lucas, Ray A.
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Newman, Jeffrey A.
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Pacifici, Camilla
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Pandya, Viraj
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Papovich, Casey
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Pérez-González, Pablo G.
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Petersen, Jayse
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Pirzkal, Nor
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Rafelski, Marc
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Ravindranath, Swara
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Simons, Raymond C.
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Snyder, Gregory F.
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Somerville, Rachel S.
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Stanway, Elizabeth R.
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Straughn, Amber N.
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Tacchella, Sandro
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Trump, Jonathan R.
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Vega-Ferrero, Jesús
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Wilkins, Stephen M.
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Yang, Guang
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Zavala, Jorge A.
Abstract
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 ∼30% at z = 6-9, while galaxies with spheroids make up ∼30%-40% across the redshift range, and pure spheroids with no evidence for disks or irregular features make up ∼20%. The fraction of galaxies with irregular features is roughly constant at all redshifts (∼40%-50%), while those that are purely irregular increases from ∼12% 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 Sérsic 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.
Volume
946
Issue
1
Start page
L15
Issn Identifier
2041-8205
Rights
open.access
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