Comparison of 3σ exomoon detection rates in warm (blue) and cold (pink) planetary systems for 120 s (solid lines) and 300 s (dashed lines) exposure cadence. Each panel corresponds to a different minimum number of confirming methods (n ≥ 1 to n ≥ 5), with detection rates shown as a function of exomoon radius. Results are presented for two stellar magnitude ranges: m_V = 6–10.5, represented by solid-colored lines, and m_V = 13.5, represented by faded lines.