collaborators

10 papers

astro-ph.HE2026

Little Red Dots as Supermassive Analogs of SS 433

Shuying Zhou, Mouyuan Sun, Xihan Ji +11

High-redshift little red dots (LRDs) are compact sources characterized by V-shaped spectral energy distributions (SEDs), broad emission lines, and often prominent Balmer breaks. Th…

astro-ph.HE2026

Revisiting the X-ray Variability Plane of AGNs: The Significant Role of the Photon Index

Ruisong Xia, Hao Liu, Yongquan Xue +9

X-ray variability provides a powerful probe of the innermost regions of active galactic nuclei (AGNs), offering valuable insights into the accretion process and the structure of th…

astro-ph.HE2026

X-ray Quasi-Periodic Oscillations in Active Galactic Nuclei and Their Implications for the Changing Look Phenomenon

Mouyuan Sun, Shuying Zhou, Jihong Liu +12

X-ray timing of active galactic nuclei (AGN) provides a unique probe of gas accretion onto supermassive black holes (SMBHs). Quasi-periodic oscillations (QPOs), which trace gas dyn…

astro-ph.HE2026

Illuminating the Mass Gap Through Deep Optical Constraint on a Neutron Star Merger Candidate S250206dm

Zhengyan Liu, Zelin Xu, Ji-an Jiang +35

The gravitational wave (GW) event S250206dm, as the first well-localized neutron star merger candidate potentially located in the mass gap, presented a unique opportunity to probe…

astro-ph.HE2025

Which active galaxies might be neutrino emitters?

Shuying Zhou, Mouyuan Sun, Guobin Mou +4

The IceCube Neutrino Observatory has identified several individual neutrino emitters associated with supermassive black hole accretion phenomena, including blazars, tidal disruptio…

astro-ph.HE2025

Multiwavelength Observations of the Apparently Non-repeating FRB 20250316A

Ye Li, Hui Sun, Lei Qian +72

The physical origin of fast radio bursts (FRBs) remains uncertain. Although multiwavelength observations have been widely conducted, only Galactic FRB~20200428D is associated with…