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emission-spectroscopy

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Ultra-hot Jupiter study combining real TESS transits with multiple JWST dayside-spectrum reductions to examine thermal inversion, water emission, extreme irradiation and reduction-to-reduction consistency.

  • Updated Oct 14, 2026
  • Python

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.

  • Updated Oct 14, 2026
  • Python

Highly inflated hot-Jupiter study combining a corrected TESS transit with three independent JWST/NIRISS dayside-emission reductions to examine water emission and reduction consistency.

  • Updated Oct 14, 2026
  • Python

Warm-Jupiter atmosphere study combining real TESS transit analysis with public JWST transmission and emission spectra to audit methane chemistry, water models and evidence across both observing geometries.

  • Updated Oct 14, 2026
  • Python

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