Report on GJ 1214 b: a JWST MIRI phase-curve spectrum inverted to per-bin brightness temperature, with propagated uncertainties, compared against Kempton et al. (2023)'s own published values.
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Aug 15, 2026 - HTML
Report on GJ 1214 b: a JWST MIRI phase-curve spectrum inverted to per-bin brightness temperature, with propagated uncertainties, compared against Kempton et al. (2023)'s own published values.
Report on WASP-121 b: a JWST phase-resolved emission spectrum, with each brightness-temperature point's own posterior uncertainty propagated into the day-night contrast.
WASP-43 b: reproducible TESS transit fitting and phase-resolved JWST/MIRI spectroscopy mapping a hot Jupiter from dayside to nightside.
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