[2405.11750] The Intermediate-Mass Black Hole Reverberation …
May 20, 2024 · View a PDF of the paper titled The Intermediate-Mass Black Hole Reverberation Mapping Project: Initial Results for a candidate IMBH in a nearby Seyfert 1 Galaxy, by Wenwen Zuo and 27 other authors
Wenwen Zuo's research works | Chinese Academy of Sciences, …
Wenwen Zuo's 24 research works with 1,318 citations and 1,495 reads, including: C iv Emission-line Properties and Uncertainties in Black Hole Mass Estimates of z ∼ 3.5 Quasars
[2412.10752] Spectral Energy Distribution Variability of the Blazar …
Dec 14, 2024 · View a PDF of the paper titled Spectral Energy Distribution Variability of the Blazar OJ 287 during 2009-2021, by Wenwen Zuo and 13 other authors
An ultraluminous quasar with a twelve-billion-solar-mass black ... - Nature
Feb 25, 2015 · Here we report the discovery of an ultraluminous quasar, SDSS J010013.02+280225.8, at redshift z = 6.30. It has an optical and near-infrared luminosity a few times greater than those of...
Wenwen ZUO (0000-0002-4521-6281) - ORCID
Jul 1, 2014 · Wenwen ZUO University of Arizona: Tucson, AZ, US 2012-10-01 to 2013-11-01 | visiting scholar (Steward Observatory)
The Intermediate-Mass Black Hole Reverberation Mapping Project: …
May 20, 2024 · | First 5 Authors: Wenwen Zuo, Hengxiao Guo, Jingbo Sun, Qi Yuan, Paulina Lira | Summary: To investigate the short-term variability and determine the size of the optical continuum emitting size of intermediate-mass black holes (IMBHs), we carried out high-cadence, multi-band photometric monitoring of a Seyfert 1
Wenwen Zou - INSPIRE-HEP
Sep 14, 2023 · Wenwen Zuo, Jinyi Yang, Qian Yang, Feige Wang (Jul, 2012) Published in: Astron.J. 146 (2013) 100 • e-Print: 1207.0204 [astro-ph.CO] pdf DOI cite claim. reference search 1 citation. Discovery of six high-redshift quasars with the Lijiang 2.4m telescope and MMT #10. Xue-Bing Wu, Wen-Wen Zuo, Qian Yang, Weimin Yi, Chenwei Yang.
Optical Continuum Reverberation Mapping of a Candidate IMBH …
May 20, 2024 · | First 5 Authors: Wenwen Zuo, Hengxiao Guo, Jingbo Sun, Qi Yuan, Paulina Lira | Summary: To investigate the short-term variability and determine the size of the optical continuum emitting region of intermediate-mass black holes (IMBHs), we carried out high-cadence, multiband photometric monitoring of a Seyfert 1
Wenwen Zuo 1,Xue-BingWu1,∗,Yi-QingLiu1 & Cheng-Liang Jiao2 1Department of Astronomy, Peking University, Beijing 100871, China. 2Korea Astronomy and Space Science Institute, Daejeon, South Korea. ∗e-mail: [email protected] Abstract. Optical variability is an important feature of quasars. Taking
The evolution of chemical abundance in quasar broad line region
Jul 5, 2018 · We propose a possibility that the high metallicity in quasar BLR might be caused by metal enrichment from massive star formation in the nucleus region of quasars or even the accretion disc. Quasars are the most luminous subclass of active galactic nuclei.