Fig. 13
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Feasibility of TOI-5720 b, TOI-6008 b, and TOI-6086 b for transmission and emission spectroscopy studies. Transmission spectroscopy metric (TSM, top panel) and emission spectroscopy metric (ESM, bottom panel) as a function of planetary radius. Our planets are compared to the Earth-sized (Rp < 1.5 R⊕) known transiting exoplanets observed or scheduled on JWST around M dwarfs (Teff < 3800). The size of the points scales with the stellar radius. The points are colored according to the effective stellar temperature. The blue circles highlight our planets TOI-5720 b, TOI-6008 b, and TOI-6086 b.
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