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The geometric probability was calculated with the following formula:

$ P = \frac{R_* + R_p}{a(1-e^2)}\frac{1}{1-e \cos(\pi - \omega)} $

If the parameters were unknown, the following values were used:

$ R_* = R_{sun} $

$ R_p = R_{jup} $

$ e = 0 $

$ \omega = 0 $

If a was unknown, the geometric transit probability was left blank.