Hot Exoplanet Atmospheres Resolved with Transit Spectroscopy (HEARTS) - VIII. Nondetection of sodium in the atmosphere of the aligned planet KELT-10b

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Fig. 9

Same as Fig. 8, but in the region of H α. The color-coding is the same as in Fig. 8. The additional red line is a continuum of one equivalent height. No detection is visible in this region either, with corresponding 3σ and 5σ limits on the plot.

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