A Close Look at Lyα Emitters with JWST/NIRCam at z ≈ 3.1

A Close Look at Lyα Emitters with JWST/NIRCam at z ≈ 3.1

We study 10 spectroscopically confirmed Ly α emitters (LAEs) at z ≈ 3.1 in the Ultra Deep Survey field, covered by the James Webb Space Telescope/NIRCam in the Public Release Imaging for Extragalactic Research program. All LAEs are detected in all NIRCam bands from F090W to F444W, corresponding to r...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:The Astrophysical journal 2024-05, Vol.966 (2), p.210
Hauptverfasser: Liu, Yixiao, Dai, Y. Sophia, Wuyts, Stijn, Huang, Jia-Sheng, Jiang, Linhua
Format: Artikel
Sprache:eng
Schlagworte:
Asymmetric structures
Dwarf galaxies
Emission lines
Emitters
Galaxy evolution
Galaxy formation
Galaxy stellar content
Galaxy structure
High-redshift galaxies
Research programmes
Scaling
Space telescopes
Star & galaxy formation
Star formation
Star formation rate
Stellar mass
Ultraviolet radiation
Wavelengths
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
Beschreibung
Zusammenfassung:We study 10 spectroscopically confirmed Ly α emitters (LAEs) at z ≈ 3.1 in the Ultra Deep Survey field, covered by the James Webb Space Telescope/NIRCam in the Public Release Imaging for Extragalactic Research program. All LAEs are detected in all NIRCam bands from F090W to F444W, corresponding to rest frame wavelengths of 2200 Å to 1.2 μ m. Based on morphological analysis of the F200W images, three out of the 10 targets are resolved into pair-like systems with separations of
ISSN:0004-637X
1538-4357
DOI:10.3847/1538-4357/ad3822