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Characterizing the Origins of the Optical Variability of Radio-quiet Active Galactic Nuclei Detected by the Swift Burst Alert Telescope

  • 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, Ting-Feng Yi, 庭丰 易

Yongyun Chen et al 2026 The Astrophysical Journal Supplement Series 285 .

  • Provider: AAS Journals

Caption: Figure 4.

Relation between variability amplitude and Eddington ratio for radio-quiet AGNs. (a) Radio-quiet AGNs. (b) Radio-quiet AGNs with efficient accretion. (C) Radio-quiet AGNs with inefficient accretion. Red dots represent sources with efficient accretion, while blue dots denote those with inefficient accretion. The shaded gray regions correspond to 1σ confidence bands. The solid line indicates the best-fit relation.

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