$Galaxy Morphology from $z\sim6$ through the eyes of JWST$

Galaxy Morphology from $z\sim6$ through the eyes of JWST

We analyze the Near Infrared ($\sim0.8-1\mu$m) rest-frame morphologies of galaxies with $\log M_*/M_\odot>9$ in the redshift range $010.5$) being predominantly bulge-dominated.

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Bibliographische Detailangaben
Hauptverfasser:	Huertas-Company, M, Iyer, K. G, Angeloudi, E, Bagley, M. B, Finkelstein, S. L, Kartaltepe, J, Sarmiento, R, Vega-Ferrero, J, Haro, P. Arrabal, Behroozi, P, Buitrago, F, Cheng, Y, Costantin, L, Dekel, A, Dickinson, M, Elbaz, D, Grogin, N. A, Hathi, N. P, Holwerda, B. W, Koekemoer, A. M, Lucas, R. A, Papovich, C, Pérez-González, P. G, Pirzkal, N, Seillé, L-M, de la Vega, A, Wuyts, S, Yang, G, Yung, L. Y. A
Format:	Artikel
Sprache:	eng
Schlagworte:	Physics - Astrophysics of Galaxies Physics - Cosmology and Nongalactic Astrophysics
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Beschreibung
Zusammenfassung:	We analyze the Near Infrared ($\sim0.8-1\mu$m) rest-frame morphologies of galaxies with $\log M_*/M_\odot>9$ in the redshift range $010.5$) being predominantly bulge-dominated.
DOI:	10.48550/arxiv.2305.02478