The active galactic nucleus (AGN) accretion disks are ideal sites for hierarchical black hole (BH) mergers. To robustly probe such a possibility, we analyze binary black hole mergers in the GWTC-4 with a flexible mixture population model for component masses, spin magnitudes, and spin tilt angles, and identify two distinct subpopulations. In the second subpopulation characterized by high spin magnitudes $\chi \sim 0.8$ as well as the broad mass distribution up to $\gtrsim 150M_{\odot }$, we find a pronounced preference for spins aligned with the orbital angular momentum: an isotropic tilt distribution is strongly disfavored (logarithmic Bayes factor $=4.5$). The aligned events account for $\sim 0.57_{-0.31}^{+0.23}$ of the second subpopulation, corresponding to a local rate of $\sim 0.25_{-0.16}^{+0.38}{\mathrm{Gpc}}^{-3}{\mathrm{yr}}^{-1}$ (all values reflect central 90% credible intervals). These notable features naturally arise from hierarchical mergers embedded in AGN disks, where gas torques may effectively align spins. Our results suggest that AGN-disk hierarchical assembly may be one important channel for the present gravitational-wave sample, and provide concrete, testable predictions for future detection.

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• Gravitational wave sources
• Gravitational waves
• Accretion disk & black-hole plasma
• Astronomical black holes
• Galactic nuclei & quasars