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Fig. B.1.

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Hertzsprung-Russell diagram similar to Fig. 3 but including only the 216 stars from our Gaia-detected sample having TESS light curves. Each star is colour-coded according to its light curve shape and content in the Fourier domain with purple indicating mono-periodic stars, olive multi-periodic, and red hybrid pulsators. The stars classified as other are shown in cyan and are discussed in the main text.

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