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Major Galaxy Mergers Only Trigger the Most Luminous Active Galactic Nuclei

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Figure

Figure 1 shows the fraction of AGNs showing mergers as a function of bolometric luminosity, which increases rapidly, from
Figure 2. Spectral energy distribution of the extragalactic X-ray “background”
Figure 3. Left panel: cumulative number of merger-triggered AGNs relative to the total number of AGNs as a function of redshift

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