activity
20182022
most citedOn the Observational Difference Between the Accretion Disk-Corona Connections among Super- and Sub-Eddington Accreting Active Galactic Nuclei

65 citations · 185 across the 7 of their papers we have counts for

collaborators

8 papers

astro-ph.HE202217 cited

A Rapid and Large-Amplitude X-ray Dimming Event in a z ~ 2.6 Radio-Quiet Quasar

Hezhen Liu, B. Luo, W. N. Brandt +4

We report a dramatic fast X-ray dimming event in a z=2.627 radio-quiet type 1 quasar, which has an estimated supermassive black hole (SMBH) mass of . In t…

astro-ph.GA2021

Reverberation Mapping of Two Luminous Quasars: the Broad-line Region Structure and Black Hole Mass

Sha-Sha Li, Sen Yang, Zi-Xu Yang +21

We report the results of a multi-year spectroscopic and photometric monitoring campaign of two luminous quasars, PG~0923+201 and PG~1001+291, both located at the high-luminosity en…

astro-ph.GA202165 cited

On the Observational Difference Between the Accretion Disk-Corona Connections among Super- and Sub-Eddington Accreting Active Galactic Nuclei

Hezhen Liu, B. Luo, W. N. Brandt +5

We present a systematic X-ray and multiwavelength study of a sample of 47 active galactic nuclei (AGNs) with reverberation-mapping measurements. This sample includes 21 super-Eddin…

astro-ph.HE202042 cited

The frequency of extreme X-ray variability of radio-quiet quasars

John D. Timlin, W. Niel Brandt, Shifu Zhu +3

We analyze 1598 serendipitous Chandra X-ray observations of 462 radio-quiet quasars to constrain the frequency of extreme amplitude X-ray variability that is intrinsic to the quasa…

astro-ph.GA20201 cited

On the Fraction of X-ray Weak Quasars from the Sloan Digital Sky Survey

Xingting Pu, B. Luo, W. N. Brandt +4

We investigate systematically the X-ray emission from type 1 quasars using a sample of 1825 Sloan Digital Sky Survey (SDSS) non-broad absorption line (non-BAL) quasars with Chandra…

astro-ph.GA202034 cited

An Extreme X-ray Variability Event of a Weak-Line Quasar

Qingling Ni, W. N. Brandt, W. Yi +8

We report the discovery of an extreme X-ray flux rise (by a factor of > 20) of the weak-line quasar SDSS J153913.47+395423.4 (hereafter SDSS J1539+3954) at z = 1.935. SDSS J1539+39…