The incidence of X-ray AGN and non-AGN galaxies in the far-infrared: Insights into host galaxy properties and AGN obscuration

Open Access

Fig. 7.

SFR as a function of λ_sBHAR, for Herschel detected and no-Herschel detected X-ray AGNs. The top panel presents the results in the total redshift range, 0 < z < 2, while the bottom panel presents the measurements when we split the X-ray AGNs sample into two redshift bins.

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