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This course aims to explore new capabilities in numerical relativity with a focus on binary black holes. The learning outcomes include understanding the advancements in gravitational wave astrophysics, improvements in numerical codes for black holes, and enhancements in computational algorithms. The course teaches skills such as gravitational wave extraction, implementing new computational algorithms, conducting longer simulations, and expanding parameter space coverage. The teaching method involves a lecture format with a presentation on various dimensions of improvements in numerical relativity. This course is intended for individuals interested in gravitational wave astrophysics, computational astrophysics, and numerical simulations in astrophysics.
