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Many of these objects were likely caught into resonances by planetary migration---either smooth or stochastic---approximately 4 Gyr ago. Some, however, gravitationally scattered off of Neptune and became transiently stuck in more recent events. Here, we use numerical simulations to predict the number of transiently-stuck objects, captured from the current actively scattering population, that occupy 111 resonances at semimajor axes $a=$30--100 au. 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