Stellar flare morphology with TESS across the main sequence

Open Access

Fig. 11.

Fitted parameters for the power law in the form ED $(A, t_{1 / 2}) = α \cdot A^{β} \cdot t_{1 / 2}^{γ}$ $(A, t_{1/2}) = \alpha \cdot A^{\beta} \cdot t_{1/2}^{\gamma}$ and with the same binning as in Fig. 9. The gray area denotes the uncertainty of the fit. The dashed lines show the parameters for the analytic template of Davenport et al. (2014).

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