2026ApJ...997..297S

Starspots trace stellar magnetic activity and affect both stellar evolution and exoplanet characterization. While occultation-based spot studies have been applied to individual systems, comparative analyses remain limited. We apply the StarryStarryProcess Bayesian surface mapping framework to archival Kepler light curves of two planet hosts-Kepler-63 and Kepler-17-extending the validation established on TOI-3884 (Paper I). Across both systems, we infer characteristic spot radii of <10^∘. The latitudinal distributions of both G-dwarfs exhibit active latitudes (Kepler-63 at ±30^∘, Kepler-17 at ±15^∘). Our analysis yields stellar obliquity measurements in excellent agreement with previous studies for both systems. This validates our methodology and demonstrates that transit-based surface mapping can simultaneously recover planetary parameters, stellar orientations, and magnetic morphologies. The analysis of the systems inferred nearly aligned (Kepler-17) to highly misaligned (Kepler-63) geometries.