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Fig. 9

image

Atmospheric mass Δσ∕ΔM for the synthetic planets vs. the bulk density (left) and median atmospheric thickness (right) for different irradiation. The light green and red regions represent the ranges in which decreasing the observational uncertainties lead and do not lead to better constraints on the atmospheric mass, respectively. The blue region represents the density range in which planets with an irradiation of 100 Earth fluxes have better constrained atmospheric mass with decreasing uncertainties and planets with an irradiation of one Earth flux do not.

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