Ultra-hot Jupiter atmosphere study using phase-resolved JWST/NIRSpec G395H emission spectroscopy to measure day-night brightness-temperature contrast, with reproducible uncertainty propagation and archive-backed system context.
astronomy reproducible-research exoplanets scientific-visualization astrophysics data-analysis jwst planetary-science astronomical-data nirspec observational-astronomy brightness-temperature emission-spectroscopy nasa-exoplanet-archive phase-curve ultra-hot-jupiter exoplanet-research wasp-121b day-night-contrast
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Updated
Aug 15, 2026 - HTML