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.
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Multi-mission X-ray imaging and spectroscopy of the PWN around PSR B1853+01 reveals a hard-spectrum outflow and diffuse halo interpreted as escaping high-energy particles.
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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.
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The pulsar wind nebula around B1853+01 in X-rays
Multi-mission X-ray imaging and spectroscopy of the PWN around PSR B1853+01 reveals a hard-spectrum outflow and diffuse halo interpreted as escaping high-energy particles.