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Fig. 15
Longwave (left) and shortwave M-Earth TIR spectra. Gaussian spectral response with R ≈ 2800 (LW) and R ≈ 2400 (SW). Solid lines show the fitted model spectra. Furthermore, the noise (S∕N = 5) contaminated “observation” of GJ 551 (Proxima Centauri) is shown (red points).
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