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Table 3.

Power law fit parameters α and β for all clusters and Teff bins in EKp and ED FFDs.

αs βs [yr−1] EDmin [s] EDmax [s] ntot, s nfit, s αerg βerg [yr−1] EKp, min [erg] EKp, max [erg] ntot, erg nfit, erg
Teff Cluster
2500–3000 Hyades 1.24 × 103 1.66 × 104 26 9 1.11 × 1032 2.82 × 1033 26 13
Pleiades 0.99 × 103 1.52 × 104 23 12 1.45 × 1032 2.08 × 1033 23 12
Praesepe 1.13 × 103 0.86 × 104 9 4 2.3 × 1032 1.53 × 1033 9 4
3000–3250 Hyades 2.37 × 102 1.29 × 104 137 76 1.31 × 1032 0.84 × 1034 137 78
Pleiades 0.58 × 103 0.63 × 105 616 258 2.32 × 1032 2.11 × 1034 616 311
Praesepe 0.7 × 103 0.82 × 105 601 275 0.4 × 1033 0.36 × 1035 601 302
3250–3500 Hyades 1.37 × 102 0.36 × 104 174 83 2.04 × 1032 0.97 × 1034 174 90
Pleiades 2.19 × 102 1.62 × 104 590 310 2.95 × 1032 1.61 × 1034 590 327
Praesepe 1.59 × 102 1.03 × 104 970 612 2.28 × 1032 1.42 × 1034 970 663
Rup 147 0.67 × 102 2.81 × 102 4 4 0.9 × 1032 0.38 × 1033 4 4
3500–3750 Hyades 0.93 × 102 2.88 × 103 52 28 0.72 × 1033 1.14 × 1034 52 20
Pleiades 1.06 × 102 0.57 × 104 113 69 0.43 × 1033 0.35 × 1035 113 75
Praesepe 0.46 × 102 1.63 × 103 111 74 2.19 × 1032 0.74 × 1034 111 76
3750–4000 Pleiades 0.98 × 102 2.05 × 103 75 35 1.25 × 1033 3.03 × 1034 75 36
Praesepe 0.56 × 102 0.37 × 103 26 10 0.51 × 1033 2.95 × 1033 26 16
4000–5000 Hyades 1.22 × 101 1.1 × 102 13 7 0.48 × 1033 0.53 × 1034 13 6
Pleiades 1.17 × 102 0.46 × 104 131 55 3.06 × 1033 3.01 × 1035 131 59
Praesepe 0.99 × 101 1.52 × 103 56 47 0.52 × 1033 1.03 × 1035 56 37
5000–6000 M 67 0.6 × 102 0.6 × 102 1 1 0.62 × 1034 0.62 × 1034 1 1
Pleiades 0.34 × 102 0.6 × 103 35 19 0.5 × 1034 0.6 × 1035 35 19
Praesepe 1.49 × 101 1.85 × 102 76 42 1.68 × 1033 0.33 × 1035 76 44
Rup 147 0.56 × 102 2.16 × 102 5 4 0.61 × 1034 2.36 × 1034 5 4

Notes. This table is available at CDS. Uncertainties are given in parentheses. Indices s and erg refer to the units of ED and EKp FFDs. EKp, min/EDmin and EKp, max/EDmax are minimum and maximum detected flare ED/energy, ntot is the total number of flares in the sample. nfit is the number of flares used for the power law fit.

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