The MOPYS project: A survey of 70 planets in search of extended He I and H atmospheres - No evidence of enhanced evaporation in young planets

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Fig. 4

Transit light curve of He I triplet from TOI-1268 b detection. The He I light curve was constructed integrating the counts of the residual map in the planet rest frame around λ₀ using σ (blue) and FWHM (orange) wavelength band passes from Table I.1. The vertical lines represent the different contacts during the transit.

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