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Fig. 2.
Rest-frame 6 μm luminosity L6 μm vs. redshift z distributions for the SDSS and GAMA MIR AGNs. The solid lines indicate the running median for each group. The dashed lines mark the edges of the redshift bins for the GAMA MIR AGNs. In the same redshift range, the GAMA MIR AGNs are less powerful than the SDSS MIR AGNs.
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