Dark skies of the slightly eccentric WASP-18 b from its optical-to-infrared dayside emission

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Fig. 8

Dayside flux observed in the Spitzer/IRAC/Channel 2 passband for programmes 50517 (left panel) and 11099 (right panel). The horizontal black line and shaded areas mark the value $F_{max}^{SPITZER 2} = 3935 \pm 25 ppm$ $F_\text{max}^\text{\spitzer{}\,2}={3935}\pm{25}\,\text{ppm}$ from Table 3.

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