Image Details
Caption: Figure 5.
H ii → S → T → L → passive galaxies sequence in X-ray: the X-ray luminosities obtained via yaxx for two fitting models: (1) a power law with no intrinsic absorption and (2) a fixed power law with Γ = 1.9 with intrinsic absorption; the accretion rate values, expressed by L/ L Edd, calculated using both L bol/ L X = 16 and L bol/ L[O iii] = 600 are compared; average and median values are indicated by squares and circles, respectively.
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