Fig. 9

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Average transmission spectrum of WASP-69b in the planet rest frame in black. The blue curve is the best-fit model from the thermosphere only, while the red curve is the best-fit model from the thermosphere and exosphere. Spectra between t1 and t4 were used to built the transmission spectrum. The vertical blue dashed lines indicate the helium lines’ positions. The bump at 10 835 Å is likely due to telluric residuals.
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