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Fig. A.2

image

Measurements of Kepler-444 Ly-α line during each HST visit. We show the spectra gathered over the full HST orbits, and plotted as a function of Doppler velocity in the stellar rest frame. Subpanels display error bars typical of a full-orbit spectrum in each visit. The shaded gray area corresponds to the range affected by ISM absorption and geocoronal emission.

This figure is made of several images, please see below:

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