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Python 3 library that takes advantage of the latest SIMD (Single input multiple data) operations included in modern processors, for native vectorized optimization of analytical data processing for CTA (the Cherenkov Telescope Array).
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The aim of this project is to provide an illustrative demo on how to construct an observationally-driven population of Galactic (detached) double white dwarfs based on results derived from electromagnetic observations.
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Présentation de janvier 2023 au sein du LPC, pour l'équipe INDRA-FAZIA. Dans celle-ci, je présente les avancements de ma thèse par rapport à mon stage.
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