Fig. 14
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Predicted S/N for transmission spectroscopy observations in the V band of the known transiting exoplanets from the exoplanet.eu archive orbiting G-dwarf (or 5000 ≤ Teff ≤ 6000 K) stars, and with planetary radii and masses in the same range as TOI-1710 b (4 ≤ Rp/R⊕ ≤ 7 and 20 ≤ MP/M⊕ ≤ 40) vs. planetary radii. The S/N shown is normalized to 100 for HD 209458 b.
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