activity
20052022
most citedMid-infrared variability of changing-look AGN

148 citations · 373 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2022★ 18 cited

Discovery of a Dusty, Chemically Mature Companion to a z4 Starburst Galaxy in JWST ERS Data

Bo Peng, Amit Vishwas, Gordon Stacey +6

We report the discovery of two companion sources to a strongly lensed galaxy SPT0418-47 ("ring") at redshift 4.225, targeted by the JWST Early Release Science program. We confirm t…

astro-ph.GA2020★ 20 cited

Far-Infrared Line Diagnostics: Improving N/O Abundance Estimates for Dusty Galaxies

Bo Peng, Cody Lamarche, Gordon Stacey +8

The Nitrogen-to-Oxygen (N/O) abundance ratio is an important diagnostic of galaxy evolution since the ratio is closely tied to the growth of metallicity and the star formation hist…

astro-ph.GA2017★ 148 cited

Mid-infrared variability of changing-look AGN

Zhenfeng Sheng, Tinggui Wang, Ning Jiang +4

It is known that some active galactic nuclei (AGNs) transited from type 1 to type 2 or vice versa. There are two explanations for the so-called changing look AGNs: one is the drama…

astro-ph.HE2017★ 47 cited

Discovery of a Mid-infrared Echo from the TDE candidate in the nucleus of ULIRG F01004-2237

Liming Dou, Tinggui Wang, Lin Yan +5

We present the mid-infrared (MIR) light curves (LCs) of a tidal disruption event (TDE) candidate in the center of a nearby ultraluminous infrared galaxy (ULIRG) F01004-2237 using a…

astro-ph.GA2015★ 2 cited

Giant radio galaxies as probes of the ambient WHIM in the era of the SKA

Bo Peng, Ru-Rong Chen, Richard Strom

The missing baryons are usually thought to reside in galaxy filaments as warm-hot intergalactic medium (WHIM). From previous studies, giant radio galaxies are usually associated wi…

astro-ph2006★ 37 cited

Optical Monitoring of BL Lacertae Object OJ 287: a 40-Day Period?

Jianghua Wu, Xu Zhou, Xuebing Wu +6

We present the results of our optical monitoring of the BL Lacertae object OJ 287 during the first half of 2005. The source did not show large-amplitude variations during this peri…