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We analyzed an 6.7-year span of data from a rotating torsion-pendulum containing $\approx 10^{23}$ polarized electrons to search for the "wind" arising from ultralight, axionlike dark matter with masses between $10^{-23}$ and $10^{-18}$ eV/c$^2$.
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Ref. [ 19 ] obtained a constraint along Z, albeit with lower precision, by taking data with 4 orientations of the spin pendulum with respect to the torsion fiber, however, this was not done for the data taken for Refs. [ 20 , 21 ]
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The Rice distribution applies when the quadrature amplitudes are Gaussians with non-zero means: see https://en.wikipedia.org/wiki/Rice_distribution
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