Outflow emission from exoplanets is predicted to be most detectable in the Na I 589 nm doublet and the He* 1083 nm triplet, with HD 189733b the best candidate at a 410 ppm Na eclipse depth and SNR 2.4 per eclipse.
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Detectability of Emission from Exoplanet Outflows Calculated by pyTPCI, a New 1D Radiation-Hydrodynamic Code
Outflow emission from exoplanets is predicted to be most detectable in the Na I 589 nm doublet and the He* 1083 nm triplet, with HD 189733b the best candidate at a 410 ppm Na eclipse depth and SNR 2.4 per eclipse.