High-performance C++ framework for afterglow modeling with Python bindings. Features fast multi-wavelength light curve generation, MCMC parameter inference, and advanced physics models including shock dynamics, radiation mechanisms, and structured jets. Designed for computational efficiency and scientific workflow integration.
high-performance modeling astrophysics gravitational-waves mcmc transients jet afterglow grb neutron-star magnetar kilonova
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Updated
Sep 5, 2026 - C++