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Table 2.

Prior distributions employed for Bayesian inference across various magnitudes and distances.

Magnitude R = 1″ R = 10″ R = 20″
10 0.138 0.985 8.015
12 0.222 1.577 12.827
14 0.429 3.056 24.864
15.25 2.59 18.35 149.971
16.5 0.829 5.900 48.0

Notes. The values of the priors represent the ratio of late stars to early stars.

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