Virial black hole mass estimates of quasars in the XQ-100 legacy survey
Date Issued
2023
Author(s)
Lai, Samuel
•
Onken, Christopher A.
•
Wolf, Christian
•
Bian, Fuyan
•
•
Lopez, Sebastian
•
Abstract
The black hole (BH) mass and luminosity are key factors in determining how a quasar interacts with its environment. In this study, we utilize data from the European Southern Observatory Large Programme XQ-100, a high-quality sample of 100 X-shooter spectra of the most luminous quasars in the redshift range 3.5 < z < 4.5, and measure the properties of three prominent optical and ultraviolet broad emission lines present in the wide wavelength coverage of X-shooter: C IV, Mg II, and H β. The line properties of all three broad lines are used for virial estimates of the BH mass and their resulting mass estimates for this sample are tightly correlated. The BH mass range is log (MBH/M⊙) = 8.6–10.3 with bolometric luminosities estimated from the 3000 Å continuum in the range log (Lbol/erg s-1) = 46.7–48.0. Robustly determined properties of these quasars enable a variety of follow-up research in quasar astrophysics, from chemical abundance and evolution in the broad-line region to radiatively driven quasar outflows.
Volume
526
Issue
3
Start page
3230
Issn Identifier
0035-8711
Rights
open.access
File(s)![Thumbnail Image]()
Loading...
Name
lai2023.pdf
Description
Pdf editoriale
Size
2.57 MB
Format
Adobe PDF
Checksum (MD5)
4777cc235c585be489e6b86951e828d7