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Efficient NIRCam Selection of Quiescent Galaxies at 3 < z < 6 in CEERS

Substantial populations of massive quiescent galaxies at z ≥ 3 challenge our understanding of rapid galaxy growth and quenching over short timescales. In order to piece together this evolutionary puzzle, more statistical samples of these objects are required. Established techniques for identifying m...

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Autors principals: Arianna S. Long, Jacqueline Antwi-Danso, Erini L. Lambrides, Christopher C. Lovell, Alexander de la Vega, Francesco Valentino, Jorge A. Zavala, Caitlin M. Casey, Stephen M. Wilkins, L. Y. Aaron Yung, Pablo Arrabal Haro, Micaela B. Bagley, Laura Bisigello, Katherine Chworowsky, M. C. Cooper, Olivia R. Cooper, Asantha R. Cooray, Darren Croton, Mark Dickinson, Steven L. Finkelstein, Maximilien Franco, Katriona M. L. Gould, Michaela Hirschmann, Taylor A. Hutchison, Jeyhan S. Kartaltepe, Dale D. Kocevski, Anton M. Koekemoer, Ray A. Lucas, Jed McKinney, Rachel Nere, Casey Papovich, Pablo G. Pérez-González, Nor Pirzkal, Paola Santini
Format: Artigo
Idioma:Inglês
Publicat: IOP Publishing 2024-01-01
Col·lecció:The Astrophysical Journal
Matèries:
Quenched galaxies
High-redshift galaxies
Two-color diagrams
Accés en línia:https://doi.org/10.3847/1538-4357/ad4cea
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