activity
20242026
most citedCounting Little Red Dots at with Ground-based Surveys and Spectroscopic Follow-up

2 citations · 5 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2026★ 1 cited

Properties and Possible Physical Origins of -ray Emission in Extreme Synchrotron Blazars

Ji-Shun Lian, Jia-Xuan Li, Ze-Rui Wang +3

Extreme synchrotron blazars, characterized by a first peak in their broadband spectral energy distributions (SEDs) at frequencies exceeding Hz, often exhibit a second pea…

astro-ph.HE2025

X-ray Polarization of the High-Synchrotron-Peaked BL Lac H 1426+428

Xin-Ke Hu, Jia-Xuan Li, Yu-Wei Yu +4

We report the X-ray polarization properties of the high-synchrotron-peaked BL Lac H 1426+428, based on two-epoch observational data from the Imaging X-ray Polarimetry Explorer (IXP…

astro-ph.EP2025★ 1 cited

Discovery of a dwarf planet candidate in an extremely wide orbit: 2017 OF201

Sihao Cheng, Jiaxuan Li, Eritas Yang

We report the discovery of a dwarf planet candidate, 2017 OF201, currently located at a distance of 90 au. Its orbit is extremely wide and extends to the inner Oort cloud, with a s…

astro-ph.GA2025★ 2 cited

Counting Little Red Dots at with Ground-based Surveys and Spectroscopic Follow-up

Yilun Ma, Jenny E. Greene, David J. Setton +13

Little red dots (LRDs) are a population of red, compact objects discovered by JWST at . At , they are roughly 100 times more abundant than UV-selected quasars. However,…

astro-ph.HE2025★ 1 cited

EP250108a/SN 2025kg: A Jet-Driven Stellar Explosion Interacting With Circumstellar Material

Gokul P. Srinivasaragavan, Hamid Hamidani, Genevieve Schroeder +28

We present optical, radio, and X-ray observations of EP250108a/SN 2025kg, a broad-line Type Ic supernova (SN Ic-BL) accompanying an Einstein Probe (EP) fast X-ray transient (FXT) a…

astro-ph.HE2024

Two-Component gamma-ray Emission Spectrum and X-Ray Polarization of the Radio Galaxy Pictor A

Jia-Xuan Li, Xin-Ke Hu, Ji-Shun Lian +6

Pictor A is a -ray emitting radio galaxy and has a bright hotspot called WHS, located 4 arcmin away from the nucleus. In this work, we present an analysis of its 16-year F…

astro-ph.HE2024

Origin of the Very High Energy γ-rays in the Low-luminosity Active Galactic Nucleus NGC 4278

Ji-Shun Lian, Jia-Xuan Li, Xin-Ke Hu +4

NGC 4278, a Low-luminosity active galactic nucleus (AGN), is generally classified as a low-ionization nuclear emission line region (LINER). Recently, it has been reported to be ass…