Fig. 6
Available maria (solid lines) and highland (dashed lines) ECOSTRESS lunar hemispherical emissivities together with our emissivity spectrum (dotted-dashed line) derived from global, disk-integrated Moon measurements (blue square boxes). Our model emissivity is not very well constrained at wavelength below 4 μm (due to reflected sunlight contributions) and in the ranges 4.6–6.5 μm and 7.3–9.7 μm (due to the lack of measurements).
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