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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 6.

Comparison between our results and previous works. The blue solid curve represents the median AGN IR SEDs of our full sample. And the pink, green, and red curves are from S16, L17, and M11. The dashed and dashed–dotted curves indicate the median AGN SEDs of high- and low-luminosity sample in this work, respectively. Our median AGN IR SED is roughly consistent with that of L17 and the M11 high-luminosity AGNs within uncertainties, but significantly disagree with that of S16. The shaded regions represent available 1σ uncertainties (derived via bootstrapping).

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