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Table 1.

Free parameters in our model of inference.

Ψbulk Bulk phase-space density parameters
ak Weights of the Gaussian mixture model
σz, k, σw, k Dispersions of Gaussian mixture model
W Vertical velocity of the Sun relative to the bulk
Ψz − mask Mask in z
Amplitudes
Means
Dispersions
Ψspiral Spiral phase-space density parameters
ρh = {1, 2, 3, 4} Mid-plane matter densities
t Time since the perturbation was produced
Initial angle of the perturbation
α Relative density amplitude of the spiral

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