Fig. 8

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Planet occurrence rate for planets with MP sin(i) > 0.8 MJup in five period bins. The blue histogram and blue dots correspond to the uncorrected rate, while the light blue histogram and black dots show the rate corrected for missed planets. Errors are derived from the binomial distribution. The log-normal fit is plotted in green, while the best-fit broken power-law is shown in red with a black dotted connector illustrating the 1σ uncertainty in Pbreak.
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