Solar-like oscillations in γ Cephei A as seen through SONG and TESS - A seismic study of γ Cephei A

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Fig. 2.

Light curve of γ Cep as observed by TESS in Sectors 18, 24, 25, and 52. Here we have removed outliers and normalised the light curve as described in Sect. 3.1. The error bars in the inset show a 24 h interval. The data shown in the inset are highlighted in the main plot as green circles with black edges and error bars.

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