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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Bibliographic Details
Published in:	The Astrophysical journal Vol. 964; no. 1; pp. 95 - 110
Main Authors:	Sun, Weibin, Fan, Lulu, Han, Yunkun, Knudsen, Kirsten K., Chen, Guangwen, Zhang, Hong-Xin
Format:	Journal Article
Language:	English
Published:	Philadelphia The American Astronomical Society 01.03.2024 IOP Publishing
Subjects:	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
Online Access:	Get full text
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