activity
20242026
collaborators

8 papers

astro-ph.HE2026

Possible High-Energy Neutrino Emission from Dark Matter Annihilation in the Disrupting Dwarf Galaxy Boötes~III

Shunhao Ji, Zhongxiang Wang

We report the first search for high-energy neutrino emissions from dark matter (DM) annihilation in stellar-stream cores. Motivated by a recent gamma-ray study that proposed these…

astro-ph.HE2026

High-energy neutrino emission from the Type~IIn supernova SN~2017hcd

Shunhao Ji, Zhongxiang Wang, Litao Zhu +1

Neutrino astronomy provides another window to exploring the Universe, exemplified by the detection of a megaelectronvolt neutrino burst from the core-collapse supernova (CCSN) SN~1…

astro-ph.HE2025

An extragalactic gamma-ray binary formed in supernova 2022jli

Pengfei Zhang, Zhongxiang Wang, Shunhao Ji

On May 5 2022, a type Ic supernova (SN) explosion SN~2022jli was discovered. This SN showed additional optical emissions, which were found to exhibit 12.4-day periodic undulations…

astro-ph.HE2025

AT2022sxl: A Candidate Repeating Tidal Disruption Event in Possible Association with Two High-Energy Neutrino Events

Shunhao Ji, Zhongxiang Wang, Litao Zhu +2

We report a candidate repeating tidal disruption event (TDE), AT2022sxl, found from large-field optical survey data. Two flares with a separation time of 7.2\,yr between the…

astro-ph.HE2025

Possible Neutrino Emission from the Pulsar Wind Nebula G63.7+1.1

Shunhao Ji, Zhongxiang Wang, Dong Zheng +1

We report on our finding of an excess of neutrinos at the location of the pulsar wind nebula (PWN) G63.7+1.1. By analyzing the IceCube track-like neutrino data for…

astro-ph.GA2024

Testing Colour-magnitude Pattern as A Method in the Search for Changing-Look AGNs

Li-tao Zhu, Zhongxiang Wang, P. U. Devanand +6

We develop a simple method to search for changing-look (CL) active galactic nucleus (AGN) candidates, and conduct a test run. In this method, optical variations of AGNs are monitor…