activity
20172026
most citedDiscovery of 21 New Changing-look AGNs in Northern Sky

220 citations · 435 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2026

Testing [O II] as a Star Formation Rate Tracer in Quasar Host Galaxies

Xiaotong Feng, Xue-Bing Wu, Yuming Fu +3

The [O II] emission line is a widely used star formation rate (SFR) tracer. However, its application to type I quasars is not straightforward, because the line can be…

astro-ph.GA2026

Far-Infrared Star Formation Rates of Quasar Host Galaxies from Multiwavelength Spectral Energy Distribution Decomposition

Xiaotong Feng, Xue-Bing Wu, Yuming Fu +3

Reliable star formation rates (SFRs) are essential for studying the connection between black hole growth and quasar host galaxies. We study the far-infrared (FIR) SFRs and the host…

astro-ph.GA2025

Quasar identifications from the slitless spectra: a test from 3D-HST

Yuxuan Pang, Xue-Bing Wu, Yuming Fu +4

Slitless spectroscopy is a traditional method for selecting quasars. In this paper, we develop a procedure for selecting quasars (QSOs) using the 3D-HST G141 slitless spectra. We i…

astro-ph.GA2025

A Pilot Study for the CSST Slitless Spectroscopic Quasar Survey Based on Mock Data

Yuxuan Pang, Xue-Bing Wu, Yuming Fu +4

The wide survey of the Chinese Space Station Telescope (CSST) will observe a large field of 17,500 . The GU, GV, and GI grism observations of CSST will cover a wavele…

astro-ph.GA2023★ 17 cited

Unveiling Luminous Ly Emitters at through JWST/NIRCam Imaging in the COSMOS Field

Yuanhang Ning, Zheng Cai, Xiaojing Lin +7

We study a sample of 14 spectroscopically confirmed Ly Emitters (LAEs) in the late era of reionization (at redshift ) based on the JWST/NIRCam imaging dataset. These…

astro-ph.GA2023★ 25 cited

CatNorth: An Improved Gaia DR3 Quasar Candidate Catalog with Pan-STARRS1 and CatWISE

Yuming Fu, Xue-Bing Wu, Yifan Li +17

A complete and pure sample of quasars with accurate redshifts is crucial for quasar studies and cosmology. In this paper, we present CatNorth, an improved Gaia DR3 quasar candidate…

astro-ph.GA2022★ 38 cited

The Large Sky Area Multi-object Fiber Spectroscopic Telescope (LAMOST) Quasar Survey: Quasar Properties from Data Release Six to Nine

Jun-Jie Jin, Xue-Bing Wu, Yuming Fu +10

We report the fourth installment in the series of the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) Quasar Survey, which includes quasars observed between Sept…

astro-ph.GA2022★ 22 cited

Finding Quasars behind the Galactic Plane. II. Spectroscopic Identifications of 204 Quasars at

Yuming Fu, Xue-Bing Wu, Linhua Jiang +21

Quasars behind the Galactic plane (GPQs) are important astrometric references and valuable probes of Galactic gas, yet the search for GPQs is difficult due to severe extinction and…

astro-ph.GA2022★ 29 cited

A Systematic Analysis of Stellar Populations in the Host Galaxies of Changing-look AGNs

Jun-Jie Jin, Xue-Bing Wu, Xiao-Tong Feng

"Changing-look" active galactic nuclei (CL-AGNs) are a newly-discovered class of AGNs that show the appearance (or disappearance) of broad emission lines within a short time scale…

astro-ph.GA2021★ 34 cited

Finding Quasars behind the Galactic Plane. I. Candidate Selections with Transfer Learning

Yuming Fu, Xue-Bing Wu, Qian Yang +4

Quasars behind the Galactic plane (GPQs) are important astrometric references and useful probes of Milky Way gas. However, the search for GPQs is difficult due to large extinctions…

astro-ph.GA2018★ 50 cited

The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) Quasar Survey: the 4th and 5th Data Release

Su Yao, Xue-Bing Wu, Y. L. Ai +15

We present the Data Release 4&5 quasar catalog from the quasar survey by Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST), which includes quasars observed between…

astro-ph.GA2017★ 220 cited

Discovery of 21 New Changing-look AGNs in Northern Sky

Qian Yang, Xue-Bing Wu, Xiaohui Fan +12

The rare case of changing-look (CL) AGNs, with the appearance or disappearance of broad Balmer emission lines within a few years, challenges our understanding of the AGN unified mo…