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Fig. 3


PDF π1(ξ | I) for astrometric “lengths” ξ defined by Eq. (10). The orbits have random orientations (i,ω,Ω), random epochs τ, random eccentricities ∈ (0,1), and random values of log P ∈ (0.0,1.0). The corresponding PDF for P-orbits (i = ω = 90°) with e = 0.96 is a near delta function at ξ = 0.14.

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