Figure 3 - uploaded by Ludwik Adamowicz
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4. The sensitivity of the 3 color Sim. Diff. Imager to planets (at a very high 10 σ level of confidence) orbiting different primary star masses (0.5 or 1.0 solar masses (Mo)), ages (0.1-5 Gyr), and distances (5-50 pc). This assumes 2 hours of integration per star at the MMT 6.5m telescope.

4. The sensitivity of the 3 color Sim. Diff. Imager to planets (at a very high 10 σ level of confidence) orbiting different primary star masses (0.5 or 1.0 solar masses (Mo)), ages (0.1-5 Gyr), and distances (5-50 pc). This assumes 2 hours of integration per star at the MMT 6.5m telescope.