Infrared emission from z ∼ 6.5 quasar host galaxies: a direct estimate of dust physical properties

Quasars at the dawn of cosmic time (z > 6) are fundamental probes for investigating the early coevolution of supermassive black holes and their host galaxy. Nevertheless, their infrared spectral energy distribution currently remains poorly constrained because the photometric coverage that probes the...

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Главные авторы:	Costa M., Decarli R., Pozzi F., Cox P., Meyer R. A., Pensabene A., Venemans B. P., Walter F., Xu F.
Формат:	Artigo
Язык:	Inglês
Опубликовано:	EDP Sciences 2026-02-01
Серии:	Astronomy & Astrophysics
Предметы:	galaxies: high-redshift galaxies: ism quasars: general galaxies: star formation
Online-ссылка:	https://www.aanda.org/articles/aa/full_html/2026/02/aa56812-25/aa56812-25.html
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