activity
20232026
most citedDoes Feedback from Supermassive Blackhole Co-evolve With Host In Type 2 Quasars?

6 citations · 8 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2026

In the Eye of the Storm: The Third Giant X-ray Outburst of the Extreme Changing-look AGN IC 3599

D. Grupe, S. Komossa, W. Zheng +10

We report the discovery and multiwavelength follow-up observations of a giant (factor >100) X-ray outburst of the exceptional changing-look active galactic nucleus (AGN) IC 3599. T…

astro-ph.GA2026

OQ~208: A New Fe~II Changing-look Active Galactic Nucleus and Implications for the Nature of the Changing-look Phenomenon

J. Wang, W. K. Zheng, D. W. Xu +5

In addition to the traditional hydrogen Balmer emission lines, here we extend the optical changing-look (CL) phenomenon occurring in some active galactic nuclei (AGNs) to the optic…

astro-ph.HE2026

SDSSJ110546.07+145202.4: The first long-duration radio changing-look NLS1 galaxy

S. Komossa, D. Grupe, A. Kraus +12

SDSSJ110546.07+145202.4 stands out as a unique radio changing-look Narrow-line Seyfert 1 (NLS1) galaxy that has brightened dramatically and shows an exceptionally long duration of…

astro-ph.GA2026

Are "Changing-Look" Active Galactic Nuclei Special in the Coevolution of Supermassive Black Holes and their Hosts? II. The Case of Changing-Look Narrow-Line Seyfert 1 Galaxies

J. Wang, S. Jin, D. W. Xu +5

The evolutionary role of the so-called ``changing-look'' (CL) active galactic nucleus (AGN), which is characterized by spectral-type transitions within yr, has been sugges…

astro-ph.HE2025

Picking-up Local GRB Candidates Based on Their Host Galaxies

J. Wang, Y. Xu, L. J. Chen +4

Rapid identification of candidates of high-value gamma-ray bursts (GRBs), including both high- and local events, is crucial for outlining subsequent observational strategy. In t…

astro-ph.HE2025

Characterizing Candidate Blazar Counterparts of the Ultra-High-Energy Event KM3-230213A

KM3NeT Collaboration, MessMapp Group, LAT Collaboration +13

High-energy astrophysical neutrinos serve as crucial messengers for understanding hadronic acceleration processes and identifying the origins of cosmic rays, with blazars among the…

astro-ph.IM2025

Enhancing Fault Diagnosis in GWAC: A Monitoring System for Telescope Arrays

Y. Xu, G. W. Li, J. Wang +6

The Ground-based Wide-Angle Cameras array (GWAC) necessitates the integration of over 100 hardware devices, more than 100 servers, and upwards of 2500 software modules, all synchro…

astro-ph.SR2024

Potential Chromospheric Evaporation in A M-dwarf's Flare Triggered by Einstein Probe Mission

J. Wang, X. Mao, C. Gao +12

Although flares from late-type main-sequence stars have been frequently detected in multi-wavelength, the associated dynamical process has been rarely reported so far. Here, we rep…

astro-ph.HE2024★ 1 cited

Capability of Searching for Kilonova Associated with a Short Gamma-ray Burst by SVOM

J. Wang, L. P. Xin, Y. L. Qiu +4

In spite of the importance of studying the cosmic generation of heavy elements through the r-process, the detection of kilonova resulted from a merger of neutron star binaries is s…

astro-ph.GA2024

Instability of Circumnuclear Gas Supply as An Origin of "Changing-look" Phenomenon of Supermassive Blackholes

J. Wang, D. W. Xu, Xinwu Cao +3

The origin of the "Changing-look" (CL) phenomenon in supermassive black holes (SMBHs) remains an open issue. This study aims to shed light on this phenomenon by focusing on a sampl…

astro-ph.GA2024★ 1 cited

Changing-look NLS1 galaxies, their detection with SVOM, and the case of NGC 1566

D. W. Xu, S. Komossa, D. Grupe +15

We discuss applications of the study of the new and barely explored class of changing-look (CL) narrow-line Seyfert 1 (NLS1) galaxies and comment on their detection with the space…

astro-ph.GA2023★ 6 cited

Does Feedback from Supermassive Blackhole Co-evolve With Host In Type 2 Quasars?

S. Jin, J. Wang, M. Z. Kong +5

The feedback from accretion of central supermassive black holes (SMBHs) is a hot topic in the co-evolution of the SMBHs and their host galaxies. By tracing the large scale outflow…