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Table 4.

FFDs: Results.

Cluster Tmin Tmax n* nflares α logβ logβ2 logEmin
M 44 3000 7000 766 155 2.21 ± 0.02 40.14 ± 0.70 32.89
M 44 3000 3249 206 22 2.05 ± 0.02 34.50 ± 0.90 33.05
M 44 3250 3499 164 55 2.13 ± 0.05 37.50 ± 1.79 32.76
M 44 3500 3749 152 88 2.02 ± 0.03 34.00 ± 1.00 32.56
M 44 3750 4000 47 13 2.01 ± 0.07 33.39 ± 2.61 32.60
M 45 3000 7000 737 596 2.16 ± 0.01 39.03 ± 0.53 32.93
M 45 3000 3249 224 94 2.05 ± 0.01 34.89 ± 0.65 32.68
M 45 3250 3499 195 262 2.14 ± 0.02 38.37 ± 0.92 32.77
M 45 3500 3749 130 179 2.37 ± 0.03 46.13 ± 1.21 32.88
M 45 3750 4000 47 53 2.15 ± 0.06 39.07 ± 2.20 32.99

Notes. Power law parameters to the FFDs as in Eq. (12). n*, nflares: number of stars and flares in the respective Tmin − Tmax bins. We note that the numbers in nflares partly do not sum up, because the median flare energy thresholds in each Teff bin vary slightly. The largest bin also overlaps with the 250 K bins. β2 indicates a least-square fit with α ≡ 2. Emin designates the low-energy detection threshold derived from synthetic flare injection.

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