Under demonstrated JWST noise and ~10° obliquities, order-10 known-plus-undiscovered wide-orbit giants are favorable for single-transit oblateness or Ganymede-moon detections; red noise or low obliquity can erase the yield.
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How Many Transiting Giant Planets Can JWST Search for Moons and Rotational Oblateness?
Under demonstrated JWST noise and ~10° obliquities, order-10 known-plus-undiscovered wide-orbit giants are favorable for single-transit oblateness or Ganymede-moon detections; red noise or low obliquity can erase the yield.