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...

Ausführliche Beschreibung

Bibliografische Detailangaben

Hauptverfasser:	Costa M., Decarli R., Pozzi F., Cox P., Meyer R. A., Pensabene A., Venemans B. P., Walter F., Xu F.
Format:	Artigo
Sprache:	Inglês
Veröffentlicht:	EDP Sciences 2026-02-01
Schriftenreihe:	Astronomy & Astrophysics
Schlagworte:	galaxies: high-redshift galaxies: ism quasars: general galaxies: star formation
Online-Zugang:	https://www.aanda.org/articles/aa/full_html/2026/02/aa56812-25/aa56812-25.html
Tags:	Tag hinzufügen Keine Tags, Fügen Sie das erste Tag hinzu!