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AGNs Are Not That Cool: Revisiting the Intrinsic AGN Far-infrared Spectral Energy Distribution

  • Authors: Jun Xu, Mouyuan Sun, and Yongquan Xue

2020 The Astrophysical Journal 894 21.

  • Provider: AAS Journals

Caption: Figure 1.

Bolometric luminosity as a function of redshift for our selected PG quasars (42 sources; red open circles), the red dashed line represents the median bolometric luminosity of our sample. For comparison, we also include the AGN samples of S16 (47 sources; blue pluses), M11 (12 sources; green diamonds), and L17 (29 sources; cyan crosses).

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