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Fig. 3

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Predicted number of planets (as a function of RP and Teq) expected to be characterized in the baseline high-contrast GSMT observing scenario outlined in Sect. 3.1. The colors and the small numbers in each cell both indicate the expectation value for that combination of RP and Teq, and the histograms show the marginalized distributions. Note that the baseline scenario simulated here conservatively assumes that planets in the two smallest RP ranges occur with equal frequency (see Sects. 2.2 and 3.2).

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