Figure 12 from Supermassive Black Holes with High Accretion Rates in Active Galactic Nuclei. VIII. Structure of the Broad-line Region and Mass of the Central Black Hole in Mrk 142

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Supermassive Black Holes with High Accretion Rates in Active Galactic Nuclei. VIII. Structure of the Broad-line Region and Mass of the Central Black Hole in Mrk 142

Authors: Yan-Rong Li, Yu-Yang Songsheng, Jie Qiu, Chen Hu, Pu Du, Kai-Xing Lu, Ying-Ke Huang, Jin-Ming Bai, Wei-Hao Bian, Ye-Fei Yuan, Luis C. Ho, and Jian-Min Wang

2018 The Astrophysical Journal 869 137.

Provider: AAS Journals

Caption: Figure 12.

Posterior distributions of the major parameters of model M3 inferred from the mock data shown in Figure 11. Vertical dashed lines represent the input values for zone I (in blue) and zone II (in red). For the common parameters of zones I and II, red dashed lines represent the input values. The parameters ﹩{f}_{\mathrm{ellip}}﹩ and ﹩{f}_{\mathrm{flow}}﹩ for zones I and II have the same input values.

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