Extreme optical/MIR color-magnitude variability efficiently selects turn-on changing-look AGNs, with seven of twelve candidates spectroscopically confirmed and several linked to multi-year flares.
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Extreme color-magnitude variability: connection to changing-look AGNs
Extreme optical/MIR color-magnitude variability efficiently selects turn-on changing-look AGNs, with seven of twelve candidates spectroscopically confirmed and several linked to multi-year flares.