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@@ -36,4 +36,4 @@ A similar finding was made on HK Aqr. Also the three strongest flares have been
Looking at all results together, there is a trend that more flares occur when a more spotted stellar hemisphere is visible, than vice versa. This is mostly influenced by the results for K and G stars. The dip in the otherwise seemingly flat histogram for the results of M dwarfs dominates the overall results.
There is at the moment no explanation for the significant dip in the histogram and we doubt that it has a physical meaning.
All results will be published on github. The program will be available at \url{https://github.com/SGCMarkus/flaredetector} while the data will be available at \url{https://github.com/SGCMarkus/flaredetector\_results}. The different branches define which fitting function was used for the data, e.g. the results containing all plots which used a sine function to fit, are found in the "sine" branch on Github.
All results will be published on github. The program will be available at \url{https://gitlab.com/SGCMarkus/flaredetector} while the data will be available at \url{https://gitlab.com/SGCMarkus/flaredetector\_results}. The different branches define which fitting function was used for the data, e.g. the results containing all plots which used a sine function to fit, are found in the "sine" branch on Github.