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Discovery of a Redback Millisecond Pulsar Candidate: 3FGL J0212.1+5320
Kwan-Lok Li, Albert K. H. Kong, Xian Hou +4
We present a multi-wavelength study of the unidentified Fermi object, 3FGL J0212.1+5320. Within the 95% error ellipse, Chandra detects a bright X-ray source (i.e., F(0.5-7keV) = 1.…
On the Evolution of High-Redshift Active Galactic Nuclei
Jirong Mao, Minsun Kim
We build a simple physical model to study the high-redshift active galactic Nucleus (AGN) evolution within the co-evolution framework of central black holes (BHs) and their host ga…
Effect of spectral index distribution on estimating the AGN radio luminosity function
Zunli Yuan, Jiancheng wang, Ming Zhou +1
In this paper, we scrutinize the effect of spectral index distribution on estimating the AGN (active galactic nucleus) radio luminosity function (RLF) by a Monte Carlo method. We f…
What determines the observational differences of blazars?
Xu-Liang Fan, Jin-Ming Bai, Jirong Mao
We examine the scenario that the Doppler factor determines the observational differences of blazars in this paper. Significantly negative correlations are found between the observa…
A mixture evolution scenario of the AGN radio luminosity function
Zunli Yuan, Jiancheng Wang, Ming Zhou +1
We propose a mixture evolution scenario to model the evolution of the radio luminosity function (RLF) of steep spectrum AGNs (active galactic nuclei) based on a Bayesian method. In…