Resolving dust and Lyman α emission in a lensed galaxy at the epoch of reionization with JWST/CANUCS

Context. Lyman α (Lyα) emission is highly sensitive to dust and neutral hydrogen and is believed to be suppressed in dusty or hydrogen-rich galaxies – especially during the epoch of reionization (EoR). Yet, moderately dusty Lyα emitters (LAEs) are observed at this epoch, suggesting that complex inte...

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Auteurs principaux:	Markov V., Bradač M., Estrada-Carpenter V., Desprez G., Rihtaršič G., Judež J., Tripodi R., Sawicki M., Noirot G., Martis N., Willott C., Abraham R., Asada Y., Brammer G., Matharu J., Muzzin A., Sarrouh G. T. E., Withers S., Ferrara A., Fujimoto S., Gallerani S., Goovaerts I., Harshan A.
Format:	Artigo
Langue:	Inglês
Publié:	EDP Sciences 2026-04-01
Collection:	Astronomy & Astrophysics
Sujets:	dust extinction hii regions ism: lines and bands galaxies: evolution galaxies: high-redshift galaxies: ism
Accès en ligne:	https://www.aanda.org/articles/aa/full_html/2026/04/aa58580-25/aa58580-25.html
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