Evolution of Nonparametric Morphology of Galaxies in the JWST CEERS Field at z ≃ 0.8–3.0

Galaxy morphology is one of the most fundamental ways to describe galaxy properties, but the morphology we observe may be affected by wavelength and spatial resolution, which may introduce systematic bias when comparing galaxies at different redshift. Taking advantage of the broad wavelength coverag...

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Veröffentlicht in:	The Astrophysical journal Jg. 954; H. 2; S. 113 - 124
Hauptverfasser:	Yao, Yao, Song, Jie, Kong, Xu, Fang, Guanwen, Zhang, Hong-Xin, Chen, Xinkai
Format:	Journal Article
Sprache:	Englisch
Veröffentlicht:	Philadelphia The American Astronomical Society 01.09.2023 IOP Publishing
Schlagworte:	Astrophysics Classification Galactic evolution Galaxies Galaxy classification systems Galaxy evolution Galaxy structure High-redshift galaxies Morphology Nonparametric statistics Parameters Red shift Spatial resolution Stars & galaxies Stellar evolution
ISSN:	0004-637X, 1538-4357
Online-Zugang:	Volltext
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