A population synthesis study with a hybrid TIDE+L dynamical model predicts that the Cherenkov Telescope Array Observatory will detect roughly ten times more Galactic pulsar wind nebulae than are currently known in TeV gamma rays.
M., Del Zanna, L., & Amato, E
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Population synthesis of Galactic middle-aged pulsar wind nebulae I. Detection prospects for current and future instruments
A population synthesis study with a hybrid TIDE+L dynamical model predicts that the Cherenkov Telescope Array Observatory will detect roughly ten times more Galactic pulsar wind nebulae than are currently known in TeV gamma rays.