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Bayesian inference is central to extracting source properties and performing model selection in gravitational wave astronomy. In this talk I present a new framework for Bayesian inference, called SHARPy, based on the combination of the Sequential Monte Carlo and the No-U-Turn-Sampler. This approach enables efficient, gradient-based exploration of the parameter space while providing unbiased evidence estimates. Moreover, the JAX implementation enables efficient automatic differentiation and GPU acceleration. I will show that SHARPy performs full inference of binary black hole merger signals in about 10 minutes, achieving accuracy comparable to state-of-the-art methods.