GW241011 and GW241110 favor 2G+1G hierarchical-merger models over a fiducial 1G+1G population, with mild AGN-disk preference and one weak optical flare candidate.
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Exploring Hierarchical Merger Scenarios for GW241011 and GW241110
GW241011 and GW241110 favor 2G+1G hierarchical-merger models over a fiducial 1G+1G population, with mild AGN-disk preference and one weak optical flare candidate.