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Fig. 9

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a) Surface temperature vs. surface pressure for mixed CO2-H2O atmospheres under M-class insolation with no CO2 clouds and fixed H2O cloud coverage. Dashed and dotted lines show CO2 and H2O phase transitions, respectively. b) Planetary albedo vs. surface pressure for the same simulations as in a). In all cases optical depth is defined at the reference wavelength (1.5 μm).

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