Fig. A.2
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Comparison of the transmission spectra of our three HST visits obtained with iraclis, prose, and the method from Wakeford et al. (2019). The larger discrepancy of visit 3 for the method of Wakeford et al. (2019) (especially between 1.1 and 1.3 um) is due to the partial masking of the first orbit, whereas the other two analyses discard it.
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