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. 2021 Jan 15;7(3):eaba9428. doi: 10.1126/sciadv.aba9428

Fig. 4. Wavelengths of bands used opportunistically around gaps in the CO2 atmosphere of Venus (54).

Fig. 4

Collectively, these offer a comprehensive sampling of surface, water vapor cloud opacity, and stray light, as needed to estimate errors on surface bands. The black line is an observed nightside emission spectrum of Venus.