activity
20172026
most citedA mixture evolution scenario of the AGN radio luminosity function. II. Do low- and high-power radio-loud AGNs evolve differently?

23 citations · 41 across the 12 of their papers we have counts for

collaborators

12 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.HE2026

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

Longhua Qin, Jiancheng Wang, Chuyuan Yang +9

We present a joint multi-period analysis of axion-like particles (ALPs) using five sets of simultaneous Fermi-LAT and LHAASO observations of the TeV blazar Mrk~421. Photon-ALP osci…

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.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.HE2025

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★ 1 cited

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…

astro-ph.HE2024

The fundamental plane of blazars based on the black hole spin-mass energy

Xu Zhang, Dingrong Xiong, Quangui Gao +4

We examine the fundamental plane of 91 Blazars which include FSRQs and BL Lacs with known X-ray luminosity (), radio luminosity (), and black hole mass measurements ($M…

astro-ph.HE2023★ 3 cited

Constraints on Extragalactic Background Light using TeV Observations of BL Lacertae objects

Longhua Qin, Jiancheng Wang, Quangui Gao +5

The extragalactic background light (EBL) in the IR to UV bands partly absorbs very high energy (VHE, 100GeV) ray photons travelling over cosmological distances via pai…

astro-ph.HE2020★ 1 cited

Studies of Extragalactic Background Light with TeV BL Lac Objects

Longhua Qin, Jiancheng Wang, Quangui Gao +4

Very high energy (VHE; 100GeV) ray from cosmological distances are attenuated by the extragalactic background light (EBL) in the IR to UV band. By contrasting measured…

astro-ph.HE2017★ 6 cited

Using the Markov Chain Monte Carlo method to study the physical properties GeV-TeV BL Lac objects

Longhua Qin, Jiancheng Wang, Chuyuan Yang +3

We fit the spectral energy distributions (SEDs) of 46 GeV - TeV BL Lac objects in the frame of leptonic one-zone synchrotron self-Compton (SSC) model and investigate the physical p…

astro-ph.HE2017★ 7 cited

Constraining the redshifts of TeV BL Lac objects

Longhua Qin, Jiancheng Wang, Dahai Yan +3

We present a model-dependent method to estimate the redshifts of three TeV BL Lac objects (BL Lacs) through fltting their (quasi-) simultaneous multi-waveband spectral energy distr…

astro-ph.HE2017★ 23 cited

A mixture evolution scenario of the AGN radio luminosity function. II. Do low- and high-power radio-loud AGNs evolve differently?

Zunli Yuan, Jiancheng Wang, Ming Zhou +2

Following previous work, we further confirm that the cosmic evolution of steep-spectrum radio-loud AGNs (active galactic nuclei) can be reproduced by a simple combination of densit…