Physical Properties of Hyperluminous, Dust-obscured Quasars at z ∼ 3: Multiwavelength Spectral Energy Distribution Analysis and Cold Gas Content Revealed by ALMA

We present a UV to millimeter spectral energy distribution (SED) analysis of 16 hyperluminous, dust-obscured quasars at z ∼ 3, selected by the Wide-field Infrared Survey Explorer. We aim to investigate the physical properties of these quasars, with a focus on their molecular gas content. We decompos...

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Vydané v:	The Astrophysical journal Ročník 964; číslo 1; s. 95 - 110
Hlavní autori:	Sun, Weibin, Fan, Lulu, Han, Yunkun, Knudsen, Kirsten K., Chen, Guangwen, Zhang, Hong-Xin
Médium:	Journal Article
Jazyk:	English
Vydavateľské údaje:	Philadelphia The American Astronomical Society 01.03.2024 IOP Publishing
Predmet:	Active galactic nuclei Active galaxies Black holes Cold gas Cosmic dust Depletion Dust Galaxies High-redshift galaxies Infrared astronomy Median (statistics) Molecular gases Physical properties Quasars Radio telescopes Samples (statistical) Spectral energy distribution Star & galaxy formation Star formation Starburst galaxies Stellar mass
ISSN:	0004-637X, 1538-4357, 1538-4357
On-line prístup:	Získať plný text
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