activity
20092024
most citedEstimating Black Hole Masses in Active Galactic Nuclei Using the MgII 2800 Emission Line

223 citations · 885 across the 41 of their papers we have counts for

collaborators

41 papers

astro-ph.GA2024

Discovery of a Damped Ly Absorber in the Circumnuclear Zone of the FeLoBAL Quasar SDSS J083942.11+380526.3

Shengmiao Wu, Xiheng Shi, Nibedita Kalita +8

SDSS J083942.11+380526.3 () is a FeLoBAL quasar that exhibits visible Balmer absorption lines (H), implying a significant population. The quasar also shows an arr…

astro-ph.CO2023★ 1 cited

Estimating Photometric Redshift from Mock Flux for CSST Survey by using Weighted Random Forest

Junhao Lu, Zhijian Luo, Zhu Chen +10

Accurate estimation of photometric redshifts (photo-) is crucial in studies of both galaxy evolution and cosmology using current and future large sky surveys. In this study, we…

astro-ph.GA2022★ 9 cited

Radio observations of four active galactic nuclei hosting intermediate-mass black hole candidates: studying the outflow activity and evolution

Xiaolong Yang, Prashanth Mohan, Jun Yang +5

Observational searches for intermediate-mass black holes (IMBHs; ) include relatively isolated dwarf galaxies. For those that host active galactic nuclei (AG…

astro-ph.GA2022★ 2 cited

Broad Emission and Absorption Line Outflows in the Quasar SDSS J163345.22+512748.4

Bo Liu, Hongyan Zhou, Xinwen Shu +4

We present a detailed study of the optical and NIR emission and absorption line spectrum of the quasar SDSS J163345.22+512748.4. We discovered on the newly acquired NIR spectrum a…

astro-ph.GA2022★ 17 cited

The radio dichotomy of active galactic nuclei

Hubing Xiao, Jingtian Zhu, Liping Fu +2

The question of radio dichotomy in the active galactic nuclei (AGNs) is still in debate even it has been proposed for more than forty years. In order to solve the old riddle, we co…

astro-ph.HE2021★ 30 cited

The relativistic jet and its central engine of blazars

Hubing Xiao, Zhihao OuYang, Lixia Zhang +4

Jet origination is one of the most important questions of AGN, yet it stays obscure. In this work, we made use of information of emission lines, spectral energy distributions (SEDs…

astro-ph.GA2021★ 13 cited

Mrk 1239: a Type-2 Counterpart of Narrow-line Seyfert-1?

Xiang Pan, Hongyan Zhou, Chenwei Yang +10

We present new spectrophotometric and spectropolarimetric observations of Mrk 1239, one of the 8 prototypes that defines type-1 narrow-line Seyfert galaxies (NLS1s). Unlike the oth…

astro-ph.GA2020★ 3 cited

A Broad Absorption Line Outflow Associated with the Broad Emission Line Region in the Quasar SDSS J075133.35+134548.3

Bo Liu, Hongyan Zhou, Xinwen Shu +4

We report the discovery of unusual broad absorption lines (BALs) in the bright quasar SDSS J075133.35+134548.3 at z~1, and present a detailed study of BAL and emission lines using…

astro-ph.GA2020★ 2 cited

Ultradense Gases beyond Dusty Torus in a Partially Obscured Quasar

Zhenzhen Li, Hongyan Zhou, Lei Hao +1

The co-evolution between black holes and galaxies suggests that feedback of active galactic nuclei influence host galaxies through ejecting radiative and kinetic energies to surrou…

astro-ph.GA2019★ 9 cited

Discovery of Metastable He I* 10830 Mini-broad Absorption Lines and Very Narrow Paschen Emission Lines in the ULIRG Quasar IRAS F11119+3257

Xiang Pan, Hongyan Zhou, Wenjuan Liu +7

IRAS F11119+3257 is a quasar-dominated Ultra-Luminous InfraRed Galaxy, with a partially obscured narrow-line seyfert 1 nucleus. In this paper, we present the NIR spectroscopy of F1…

astro-ph.GA2019

Profile of and Variability in Double-Peaked Balmer Emission Lines in 3C 445

Shaohua Zhang, Hongyan Zhou, Xiheng Shi +2

We extract the multiple-epoch Balmer-line profiles of the heavily obscured quasar 3C 445 from the spectral curves in the literature, and analyze the emission-line profiles of the H…

astro-ph.GA2019★ 31 cited

Fast Inflow Directly Feeding Black Hole Accretion Disk in Quasars

Hongyan Zhou, Xiheng Shi, Weimin Yuan +21

Quasars are high-luminosity active galactic nuclei believed to be powered by accretion of interstellar matter onto a super-massive black hole (SMBH) therein. Most of the observed e…

astro-ph.GA2019★ 8 cited

SDSS J153636.22+044127.0 and its analogues: shocked outflows, not active binary black holes

Shaohua Zhang, Hongyan Zhou, Xiheng Shi +6

The binary emission-line system, particularly the binary broad-line emission system, is considered the most effective indicator of the black hole binary. A plausible example of suc…

astro-ph.GA2018★ 11 cited

A Deeply Buried Narrow-Line Seyfert 1 Nucleus Uncovered in Scattered Light

Xiang Pan, Honglin Lu, S. Komossa +13

We present spectropolarimetric and spectrophotometric observations of the peculiar active galactic nucleus (AGN) SDSS J120300.19+162443.7 (hereafter J1203+1624) at . Its…

astro-ph.GA2018★ 1 cited

A Strange EUV Emission: Scattered Continuum in the Lymann Limit Absorption Edge toward the Quasar SDSS J125903.26+621211.5?

Xiang Pan, Shaohua Zhang, Hongyan Zhou +5

We identified a peculiar proximate sub-damped Lya absorption system (sub-DLA) at z=3.234 with a neutral hydrogen column density of toward the…

astro-ph.IM2018

Design of Near Infrared Sky Brightness Monitor and Test Running at Ngari Observatory in Tibet

Qi-Jie Tang, Jian Wang, Shu-cheng Dong +16

Tibet is known as the third pole of the earth, as high as the South Pole and North Pole. The Ngari (Ali) observatory in Tibet has the advantage of plenty of photometric night, low…

astro-ph.GA2018★ 3 cited

Ultra-dense Broad-line Region Scale Outflow in Highly Reddened Quasar SDSS J145057.28+530007.6

Shaohua Zhang, Hongyan Zhou, Xiheng Shi +3

We report the discovery of highly reddening and hydrogen Balmer and metastable helium broad absorption lines in the quasar SDSS J145057.28+530007.6, based on the optical and near-i…

astro-ph.GA2018★ 5 cited

An Intercomparison Study of Two Proximate Damped Ly Systems with Residual Flux upon the Ly Absorption Trough toward Quasars

Xiaoyi Xie, Hongyan Zhou, Xiang Pan +6

In this paper, we present an intercomparison study of two quasars, SDSS J145618.32+340037.2 and SDSS J215331.50-025514.1, which have proximate damped Lya systems (PDLAs) with resid…

astro-ph.EP2017★ 16 cited

Searching for the Transit of the Earth--mass exoplanet Proxima~Centauri~b in Antarctica: Preliminary Result

Hui-Gen Liu, Peng Jiang, Xingxing Huang +21

Proxima Centauri is known as the closest star from the Sun. Recently, radial velocity observations revealed the existence of an Earth-mass planet around it. With an orbital period…

astro-ph.GA2017★ 20 cited

Quasar 2175 Å dust absorbers I: metallicity, depletion pattern, and kinematics

Jingzhe Ma, Jian Ge, Yinan Zhao +4

We present 13 new 2175 Å dust absorbers at z_abs = 1.0 - 2.2 towards background quasars from the Sloan Digital Sky Survey. These absorbers are examined in detail using data from th…

astro-ph.GA2017★ 12 cited

Reddening and He I* Absorption Lines in Three Narrow-line Seyfert 1 Galaxies

Shaohua Zhang, Hongyan Zhou, Xiheng Shi +6

We report the detection of heavy reddening and the He I* absorption lines at the AGNs' redshift in three Narrow-line Seyfert 1 galaxies: SDSS J091848.61+211717.0, SD…

astro-ph.GA2017★ 24 cited

Photoionization-driven Absorption Lines Variability in Balmer Absorption Line Quasar LBQS 1206+1052

Luming Sun, Hongyan Zhou, Tuo Ji +10

In this paper we present an analysis of absorption line variability in mini-BAL quasar LBQS 1206+1052. The SDSS spectrum demonstrates that the absorption troughs can be divided int…

astro-ph.GA2016★ 30 cited

The Redshifted Hydrogen Balmer and Metastable He I Absorption Line System in Mini-FeLoBAL Quasar SDSS J112526.12+002901.3: A Parsec Scale Accretion Inflow?

Xi-Heng Shi, Peng Jiang, Hui-Yuan Wang +4

The accretion of interstellar medium onto the central super massive black holes is widely accepted as the source of the gigantic energy released by the active galactic nuclei. But…

astro-ph.GA2016★ 14 cited

The Extreme Ultraviolet Variability of Quasars

Brian Punsly, Paola Marziani, Shaohua Zhang +2

We study the extreme ultraviolet (EUV) variability (rest frame wavelengths 500 - 920 ) of high luminosity quasars using HST (low to intermediate redshift sample) and SDSS (high…