Size - Stellar Mass Relation and Morphology of Quiescent Galaxies at \(z\geq3\) in Public \(JWST\) Fields

Size - Stellar Mass Relation and Morphology of Quiescent Galaxies at \(z\geq3\) in Public \(JWST\) Fields

We present the results of a systematic study of the rest-frame optical morphology of quiescent galaxies at \(z \geq 3\) using the Near-Infrared Camera (NIRCam) onboard \(JWST\). Based on a sample selected by \(UVJ\) color or \(NUVUVJ\) color, we focus on 26 quiescent galaxies with \(9.8

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Veröffentlicht in:arXiv.org 2024-02
Hauptverfasser: Ito, Kei, Valentino, Francesco, Brammer, Gabriel, Faisst, Andreas L, Gillman, Steven, Gomez-Guijarro, Carlos, Gould, Katriona M L, Heintz, Kasper E, Ilbert, Olivier, Jespersen, Christian Kragh, Kokorev, Vasily, Kubo, Mariko, Magdis, Georgios E, McPartland, Conor, Onodera, Masato, Rizzo, Francesca, Tanaka, Masayuki, Toft, Sune, Vijayan, Aswin P, Weaver, John R, Whitaker, Katherine E, Wright, Lillian
Format: Artikel
Sprache:eng
Schlagworte:
Color
Galactic evolution
Galaxies
Infrared cameras
Morphology
Stellar mass
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Zusammenfassung:We present the results of a systematic study of the rest-frame optical morphology of quiescent galaxies at \(z \geq 3\) using the Near-Infrared Camera (NIRCam) onboard \(JWST\). Based on a sample selected by \(UVJ\) color or \(NUVUVJ\) color, we focus on 26 quiescent galaxies with \(9.8
ISSN:2331-8422