Fig. 7
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Expected transmission spectral signal of 1 atmospheric scale height (Bento et al. 2014) versus stellar effective temperature for exo-planets with precise densities (σM/M ≤ 25% and σR/R ≤8%). The points of planets with Rossiter-McLaughlin (RM) observations are color-coded with the absolute value of their sky-projected spin-orbit angle The three new planets, TOI-615b, TOI-622b, and TOI-2641b, have been highlighted as orange stars and labeled.
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