Fig. 3
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HST/STIS NUV transmission spectrum of HD 189733 b (individual visits). The circles with error bars denote the transmission planet-to-star radius ratios from each echelle order and visit (see legend), corresponding to the best AICc fits. The colored dashed lines denote the mean value for each visit. The squares denote the XMM-Newton/UVM2 photometric measurement by King et al. (2021).
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