A simulation estimates HST recovery if the proposed Kepler-1708 moon exists. Seven of75 trials meet all requirements; conditional10±3% detectability is separate from the probability a moon exists. Optimistic systematics and JWST forecasts remain assumptions, with no independent detection or UAP claim.
Full supplied v2 manuscript; originals and simulations unverifiedA survey of70 cool giant planets reports a tentative exomoon candidate. Two transits and dependent treatments of Kepler data leave ordinary noise, blend and other-planet alternatives. Statistical planet validation and moon tests are separate; this is astronomy background, with no life or UAP detection.
Full supplied v1 manuscript; original and model checks remain openThe authors find no compelling exomoon evidence among seven selected Kepler candidates. Archival transit analysis and author-reported2012 stellar spectra support conditional mass limits; physical and predictive checks reject candidate fits. Noise, starspots and model assumptions limit inference. This provides research-method context, with no independent moon or UAP confirmation.
Complete supplied manuscript; original rendition unresolvedA curated public selection. Source review describes what was read; it does not establish that a claim is true. Our research approach