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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 5.

Dependence of our median AGN SEDs upon the choice of galaxy templates. Left panel: the median SED derived with the DH02 galaxy template library vs. that with DH14. Right panel: the median SED derived with DH14 vs. that with R09. The shaded regions indicate the interquartile ranges (i.e., between the 25th and 75th percentiles) that are estimated via bootstrapping. The three median SEDs are consistent with each other (within 2σ uncertainties), with ﹩{\chi }_{\nu }^{2}=0.86﹩ and δ = 0.22 dex between the DH14 and R09 results. The difference in IRCI is 0.39 dex.

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