Inflated hot-Jupiter transit study using real TESS photometry, timing-adjusted fitting and correlated-noise scaling, with haze/cloud and stellar-activity context kept distinct from the measured transit analysis.
astronomy reproducible-research exoplanets scientific-visualization astrophysics data-analysis clouds haze tess planetary-science stellar-activity astronomical-data transit-photometry observational-astronomy nasa-exoplanet-archive exoplanet-research hat-p-32b inflated-hot-jupiter
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Updated
Aug 15, 2026 - Python