Fig. 12

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Transmission spectroscopy metric values for known exoplanets orbiting F/G stars in less than 50 days. We only show exoplanets for which TSM > 50 for clarity as ~98% of worlds in the sample lay below this value. While TOI-411 b and c fall in the 2% of this kind of planet with TSM > 50, only TOI-411 c passes the suggested threshold of 90, joining an elite group of 15 super-Earths and sub-Neptunes orbiting Sun-like stars and amenable for spectroscopic follow-up with JWST.
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