Weak Line Quasars at High Redshift: Extremely High Accretion Rates or Anemic Broad-line Regions?
Brandt, W. N.; Strauss, Michael A.; Anderson, Scott F.; Fan, Xiaohui; Schneider, Donald P.; Trakhtenbrot, Benny; Diamond-Stanic, Aleksandar M.; Netzer, Hagai; Richards, Gordon T.; Plotkin, Richard M.; Shemmer, Ohad; Lira, Paulina
United States, Israel, Chile, Netherlands
Abstract
We present Gemini-North K-band spectra of two representative members of the class of high-redshift quasars with exceptionally weak rest-frame ultraviolet emission lines (WLQs), SDSS J114153.34+021924.3 at z = 3.55 and SDSS J123743.08+630144.9 at z = 3.49. In both sources, we detect an unusually weak broad Hβ line and place tight upper limits on the strengths of their [O III] lines. Virial, Hβ-based black hole mass determinations indicate normalized accretion rates of L/L Edd=0.4 for these sources, which is well within the range observed for typical quasars with similar luminosities and redshifts. We also present high-quality XMM-Newton imaging spectroscopy of SDSS J114153.34+021924.3 and find a hard-X-ray photon index of Γ = 1.91+0.24 -0.22, which supports the virial L/L Edd determination in this source. Our results suggest that the weakness of the broad emission lines in WLQs is not a consequence of an extreme continuum-emission source but instead due to abnormal broad emission line region properties.