Fig. C.1.
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Left panel: Sensitivity in the (q, s) space for a log-uniform distribution of synthetic planets. Centre and right panels: Detected planets from a log-uniform distribution of synthetic planets in (Mp, ap), for two different star IMFs: the Robin et al. (2003) disc stars power law (centre) and the Chabrier (2005) IMF (right). The colour-coding indicates the total number of detected stars in each bin. The contours show the detection sensitivity lines of Roman from Penny et al. (2019), with the three-detection line in cyan, assuming one planet per star.
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