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Fig. A.1
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Power spectral density for HE 0057-5959 based on TESS observations during Sector 1 and 2. The light curve from which we obtain the power spectral density is provided by the TESS Asteroseis- mic Science Operations Center (TASOC; Handberg et al. 2021; Lund et al. 2021). We find no evidence of solar-like oscillations.
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