Fig. 8
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Detection map for a Jupiter-like planet hosting a 3 R⊕ sub-Neptune-sized exomoon (system ID: simu 21), using the same methodology as Figure 6 (120 s exposures, 3σ threshold). Gray-shaded regions indicate dynamically unstable configurations, and the map illustrates the systematic application of T×Vs methods for evaluating larger exomoons with ET-like photometry.
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