TY - JOUR
T1 - Virial black hole mass estimates of quasars in the XQ-100 legacy survey
AU - Lai, Samuel
AU - Onken, Christopher A.
AU - Wolf, Christian
AU - Bian, Fuyan
AU - Cupani, Guido
AU - Lopez, Sebastian
AU - D’Odorico, Valentina
N1 - Publisher Copyright:
© 2023 The Author(s).
PY - 2023/12/1
Y1 - 2023/12/1
N2 - 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.
AB - 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.
KW - galaxies: active
KW - galaxies: high-redshift
KW - quasars: emission lines
UR - http://www.scopus.com/inward/record.url?scp=85175325497&partnerID=8YFLogxK
U2 - 10.1093/mnras/stad2994
DO - 10.1093/mnras/stad2994
M3 - Article
SN - 0035-8711
VL - 526
SP - 3230
EP - 3247
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
IS - 3
ER -