Peculiar velocity measurements constrain the parameter combination , the product of the linear growth rate and the fluctuation amplitude . Under the approximation that is a monotonic function of , this can be related to , enabling direct comparison with weak lensing and cosmic microwave background results. We exploit this by using three classes of direct-distance tracers – the Tully-Fisher relation, the fundamental plane, and Type~Ia supernovae – to infer peculiar velocities. A unified hierarchical forward model jointly calibrates each distance indicator and a linear theory reconstruction of the local Universe. This is the first consistent Bayesian analysis to combine all three major classes of distance indicators within a common framework, enabling cross-checks of systematics across diverse galaxy populations. All three tracers yield consistent values of that are also in agreement with Planck. Our joint constraint is , with the uncertainty dominated by the 2M++ galaxy field. These results demonstrate that peculiar velocity surveys provide a robust, consistent measurement of , and support concordance with the cosmic microwave background.

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