Simulated data, and aggregated results necessary to recreate the results and figures in the forthcoming paper, Ilin et al. 2023: "Flaring Latitudes in Ensembles of Low Mass Stars" (link TBD). The double timestamped files are simulated mean and standard deviation values for ensembles of randomly oriented stars, split into the training and the validation data sets. Their configurations are listed in the _all_runs file. You can find the aggregated mean and standard deviation values in _all_means_std. The flare parameter fits from Fig. 1 are under _a_from_ed and fwhm_from_ed_a. The fit parameters from Table 2 in the paper are in fit_paratemers. The results for the Okamoto et al. (2021) G dwarf flares are in okamoto2021_table.