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Fig. B.1
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Out-of-transit ESPRESSO CCF of HIP 41378 (in blue) compared with one CCF of HD 88595 (Sulis et al. 2023), a star similar in Teff to HIP 41378 with a higher υ sin(i*) = 7.24 ± 0.35 km s–1 (orange dashed line). The theoretical rotation profile of a star with υ sin(i*) = 11 km s–1 is represented as a dotted black line.
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