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This course teaches learners about a modular weak-lensing processing and analysis pipeline. The learning outcomes include understanding the importance of weak gravitational lensing in cosmology, learning how to measure the shapes of galaxies accurately, and exploring Python tools developed for this purpose. The course aims to equip participants with the skills to work with ShapePipe, a Python-based solution for analyzing weak lensing data. The teaching method involves a presentation by Samuel Farrens, showcasing the tools developed and their applications in cosmological research. This course is intended for Python programmers, cosmologists, and individuals interested in scientific software development.