Fraction of passive vs. active spiral host galaxies in the main sample of x-ray AGN in clusters comparing with both the control samples, with cluster galaxies and with x-ray AGN from the field. The classification has been made based on visual inspection from the HSC images. The sample is statistically small but there is a clear trend, specifically in the case of the x-ray AGN in clusters we find only passive spiral AGN host galaxies and found up to 2r₅₀₀ cluster region. Error bars indicate the 1σ confidence limits for small numbers of events (Gehrels 1986).