activity
20242026
collaborators

8 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.GA2026

The Large Sky Area Multi-object Fiber Spectroscopic Telescope (LAMOST) Quasar Survey: Quasar Properties from Data Release 10 to 12

Bing Lyu, Xue-Bing Wu, Jun-Jie Jin +9

We present the quasar catalog from Data Releases 10 to 12 of the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) Quasar Survey, comprising quasars observed betwe…

astro-ph.GA2025

Systematic Analysis of Changing-look AGN Variability Using ZTF Light Curves

Huimei Wang, Xue-Bing Wu, Nanyu Yao +5

Changing-look active galactic nuclei (CLAGNs) are a unique population of AGNs that exhibit the appearance (turn-on) or disappearance (turn-off) of broad emission lines. This study…

astro-ph.GA2025

The CatSouth Quasar Candidate Catalog for the Southern Sky and a Unified All-Sky Catalog Based on Gaia DR3

Yuming Fu, Xue-Bing Wu, R. J. Bouwens +12

The Gaia DR3 has provided a large sample of more than 6.6 million quasar candidates with high completeness but low purity. Previous work on the CatNorth quasar candidate catalog ha…

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…