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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 9.

Top left: an example of a transfer function obtained using model M3. Top right: comparison of velocity-binned time lags obtained from model M3 and CCF analysis. Bottom left: delay integral of the transfer function ﹩{\rm{\Psi }}(v)﹩, superposed on the observed, scaled mean Hβ profile. Shaded areas represent the 1σ error band. Bottom right: velocity integral of the transfer function ﹩{\rm{\Psi }}(\tau )﹩. Shaded areas represent the 1σ error band. The dashed line represents the CCF between the observed light curves of the continuum and Hβ fluxes.

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