collaborators

6 papers

astro-ph.CO2026

Shape-Preserving Evolution of the Global Ultraviolet Quasar Luminosity Function to

Wenjie Wang, Zunli Yuan, Yu Luo +1

We present a global unbinned-likelihood analysis of the rest-frame ultraviolet (UV) quasar luminosity function (QLF) over , using a final analysis sample of 70,960…

astro-ph.IM2026

A flexible method for estimating luminosity functions via Kernel Density Estimation -- III. Extending to Multiple Flux-Limited Samples

Zunli Yuan, Chuanqi Li, Wenjie Wang +2

As the third paper in a series regarding the estimation of luminosity functions (LFs) via kernel density estimation (KDE), we present a further generalization of our framework by e…

astro-ph.HE2026

Joint Multi-Period Fermi-LAT and LHAASO Constraints on Axion-Like Particles from Mrk 421 Using Profile Likelihood with Gaussian Copula Correlation

Longhua Qin, Jiancheng Wang, Chuyuan Yang +8

We propose a joint multi-epoch profile-likelihood analysis of axion-like particles (ALPs) using five sets of simultaneous Fermi-LAT and LHAASO observations of the TeV blazar Mrk 42…

astro-ph.IM2026

CosmicWeb-21cm array: A New Radio Observation Array Design for 21cm Cosmology

Jiancheng Wang, Jirong Mao, Xiangming Cheng +10

This paper presents the CosmicWeb-21cm array, a novel radio interferometer designed to overcome the key challenges in 21 cm cosmology. Its core innovations include: (1) a multi-sca…

astro-ph.HE2026

Revisiting Very High Energy Gamma-Ray Absorption in Cosmic Propagation under the Combined Effects of Axion-Like Particles and Lorentz Invariance Violation

Longhua Qin, Jiancheng Wang, Chuyuan Yang +9

Very-high-energy (VHE; GeV) gamma rays are expected to experience strong attenuation during cosmological propagation due to electron-positron pair production on the…

astro-ph.GA2025

Optical Monitoring and Long-term Optical Spectral Variability of BL Lacertae Object S5 0716+714

Huai-Zhen Li, Di-Fu Guo, Long-Hua Qin +7

We present photometric observations of the BL Lacertae object S5 0716+714 with a temporal resolution of 120 s in the Sloan i' and r' bands. These observations were conducted using…