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Characterizing the Origins of the Gamma-Ray Variability of the Jetted Active Galactic Nuclei Observed with Fermi-LAT

  • Authors: Yongyun Chen, 永云 陈, Qiusheng Gu, 秋生 顾, Junhui Fan, 军辉 樊, Dingrong Xiong, 定荣 熊, Xiaoling Yu, 效龄 俞, Xiaogu Zhong, 晓谷 钟, Xiaotong Guo, 晓通 郭, Nan Ding, 楠 丁

Yongyun Chen et al 2026 The Astrophysical Journal Supplement Series 284 .

  • Provider: AAS Journals

Caption: Figure 5.

(a) The relation between the amplitude of variability and radio luminosity; (b) the relation between the amplitude of variability and 0.3–10 keV X-ray luminosity; (c) the relation between the amplitude of variability and gamma-ray luminosity; (d) the relation between the amplitude of variability and radio loudness; (e) the relation between the amplitude of variability and X-ray loudness; and (f) the relation between the amplitude of variability and gamma-ray loudness. The red dots are FSRQs. The blue dots are BL Lacs. The green dots are BCUs. The cyan dots are NLS1s. The shaded gray colored areas correspond to 1σ confidence bands. The black line is the best fit.

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