Table B.1
Gaussian prior for the MCMC-approach for the MuSCAT instruments.
| Parameter | M1 and M2 |
|---|---|
| tpeak | N(tpeak, d) |
| amflare | N(amrec, 0.05) |
| FWHMflare | N(FWHMest,  d) |
| Teff | U(log(Teff), 3.3,4.4K) |
| a | U(log(a), −10, 0) |
amrec refers here to the recorded amplitude given by Altaipony and is given in terms of normalized flux. We use all filters with the same standard deviations. For the MCMC-fits of the SEDs, we use uniform priors for the effective temperature Teff and the fraction of flaring area a in logarithmic space.
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