HR 10 as seen by CHEOPS and TESS - Revealing δ Scuti pulsations, granulation-like signal and hint for transients

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Fig. 1.

Reduced TESS lighcurves. Top: lightcurve from S2 processed following the recipe of Nardiello et al. (2020, 2021) on the SAP lightcurve (see text). Bottom: same as the top panel but for S29. The typical error on the relative flux is 10⁻⁶%, for a maximum variation of ∼0.8% of the mean brightness of the star.

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