Fig. 8
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Transmission spectra of HAT-P-67 b for each night. The spectra are centred around the Hα line in the planetary rest frame (light grey) and also binned 20 times (in black circles). The red line is the MCMC Gaussian fit performed by SLOPpy, while the vertical blue dashed line indicates the rest frame transition wavelength of the Hα line.
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