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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Veröffentlicht in:	The Astrophysical journal 2024-07, Vol.970 (1), p.68
Hauptverfasser:	Long, Arianna S., Antwi-Danso, Jacqueline, Lambrides, Erini L., Lovell, Christopher C., de la Vega, Alexander, Valentino, Francesco, Zavala, Jorge A., Casey, Caitlin M., Wilkins, Stephen M., Yung, L. Y. Aaron, Arrabal Haro, Pablo, Bagley, Micaela B., Bisigello, Laura, Chworowsky, Katherine, Cooper, M. C., Cooper, Olivia R., Cooray, Asantha R., Croton, Darren, Dickinson, Mark, Finkelstein, Steven L., Franco, Maximilien, Gould, Katriona M. L., Hirschmann, Michaela, Hutchison, Taylor A., Kartaltepe, Jeyhan S., Kocevski, Dale D., Koekemoer, Anton M., Lucas, Ray A., McKinney, Jed, Nere, Rachel, Papovich, Casey, Pérez-González, Pablo G., Pirzkal, Nor, Santini, Paola
Format:	Artikel
Sprache:	eng
Schlagworte:	Color Galactic evolution Galaxies Galaxy distribution High-redshift galaxies Populations Quenched galaxies Spectral energy distribution Star & galaxy formation Star formation Stars & galaxies Statistical analysis Statistical sampling Two-color diagrams
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