collaborators

10 papers

astro-ph.GA2026

SDSS J153231.80+420342.7: a triple black hole candidate with a close binary black hole

Qi Zheng, YiWen Jiang, Xue-Guang Zhang +1

We report a triple black hole candidate with a close binary black hole (BBH) in the blue quasar SDSS J153231.80+420342.7 (=SDSS J1532) at a redshift of 0.209. It shows double-peake…

astro-ph.GA2026

Spectroscopic study of the broad component of [O III]λ5007 profile in type 1 AGNs

Qi Zheng, Yansong Ma, Xueguang Zhang +1

The spectra of type 1 active galactic nuclei (AGNs) often exhibit broad component in [O III]5007, which are typically blue-shifted and associated with strong outflows. We system…

astro-ph.GA2025

Dual core system candidates: a sample of objects with large velocity offset between absorption and narrow emission lines

Zheng Qi, Zhang Xueguang, Yuan Qirong

We present a sample of 28 objects at z<0.3 from Data Release 16 of the Sloan Digital Sky Survey (SDSS DR16) with large velocity offset (> 200 km/s) of narrow H and H emission…

astro-ph.GA2025

AGN-Driven Biconical Outflows as the Origin of the Double-Peaked [O~{\sc iii}] doublet in SDSS J134733.36+121724.27

PeiZhen Cheng, XingQian Chen, GuiLin Liao +4

In this manuscript, we recheck the spectroscopic properties of SDSS J134733.36+121724.27 (4C+12.50), confirming the presence of the double-peaked [O~{\sc iii}]Å…

astro-ph.GA2025

On type 1 active galactic nuclei with double-peaked [O~{\sc iii}]. II. properties of long-term optical variability

Qi Zheng, Xingyv Zhu, Xueguang Zhang +1

Double-peaked \oiii~profiles could potentially indicate kiloparsec-scale dual AGNs. We analyze long-term optical light curves of 35 type 1 AGNs with such features from our recent c…

astro-ph.GA2025

A gravitational acceleration model to explain the double-peaked narrow emission lines shifted in the same direction

XingQian Chen, GuiLin Liao, Qi Zheng +1

In this manuscript, we propose, for the first time, an oversimplified but potentially effective gravitational acceleration model to interpret the double-peaked narrow emission line…

astro-ph.GA2025

An improved Seyfert-LINER classification line in the [N~{\sc ii}] BPT diagram

PeiZhen Cheng, XingQian Chen, GuiLin Liao +3

In this manuscript, an improved Seyfert-LINER classification line (= S-L line) is proposed in the [N~{\sc ii}] BPT diagram, based on a sample of 47,968 low redshift narrow emission…

astro-ph.GA2025

Optical QPOs with dual periodicities 1103days and 243days in the blue quasar SDSS J100438.8+151056

GuiLin Liao, XingQian Chen, Qi Zheng +2

This manuscript investigates the possible existence of a binary supermassive black holes (BSMBH) system in the blue quasar SDSS J100438.8+151056 (=SDSS J1004+1510) at z=0.219 based…

astro-ph.GA2025

The orbital kinematics of kpc-scale dual-core systems with double-peaked narrow emission lines

XingQian Chen, Peizhen Cheng, Ying Gu +3

In this manuscript, based on SDSS photometry and spectroscopy, a method is proposed to test the hypothesis that the orbital kinematics of kpc-scale dual-core systems can lead to do…

astro-ph.GA2025

On type 1 active galactic nuclei with double-peaked [O~{\sc iii}]. I. data sample and basic results

Qi Zheng, Yansong Ma, Xueguang Zhang +2

Double-peaked narrow emission lines (DPNELs) might be evidence for the existence of kpc-scale dual AGNs. There are so far large samples of objects with DPNELs in narrow emission li…