Fig. 8.

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SFR as function of the AGN bolometric luminosity for the [Ne V]-selected AGNs (red circles). The average SFR in three bins of SFR is reported in orange, with the error bar representing the 16th and 84th percentiles. The green points are the average SFR for the sample of X-ray and IR -selected AGNs of Stemo et al. (2020), while the cyan symbols represent those from Rosario et al. (2012, 2013), Stanley et al. (2015), Bernhard et al. (2016) collected by Bernhard et al. (2018). The black line is the prediction from their mass-dependent model.
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