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Jet Power, Bulk Lorentz Factor, Black Hole Spin, and Magnetic Field of Accretion Disk in Jetted Active Galactic Nuclei: A Large Gamma-Ray Emission Sample

  • Authors: Dingrong Xiong, Junhui Fan, Feng Yuan, Jun-Xian Wang, Minfeng Gu, Yongquan Xue, Jirong Mao, Liang Chen, Rui Xue, Xu-Liang Fan, Yongyun Chen, Nan Ding, Fei Guo, Jia-Wen Li, Dahai Yan, Y. G. Zheng, Jinming Bai

Dingrong Xiong et al 2026 The Astrophysical Journal 1009 .

  • Provider: AAS Journals

Caption: Figure 2.

The relationship between jet radiative power and intrinsic gamma-ray luminosity, with black circles representing blazars, and red circles indicating radio galaxies (RDGs). The blue solid line shows the best-fit linear model obtained via OLS fitting; the blue shaded area corresponds to the 2σ confidence band, while the gray region depicts the 2σ prediction band. The correlation coefficient for this fit is r = 0.94 (20σ significance), with a scatter of 0.05 dex.

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