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Table E.3.

Stars for which we calculated the emission measure-weighted coronal temperatures kTwgt. Because only the ratio between EM of each component matters for calculating kTwgt, they are listed as unitless in the table.

GJ 551C (quiescence) GJ 551C (flare) GJ 729 GJ 674 GJ 1245B* GJ 876 (low) GJ 876(high)
SpT M5.5 M3.5 M2 M5.5 M4
distance [pc] 1.3 3.0 4.6 4.7 4.7
kT1 [keV] 0.14 0.14 0.15 0.12 0.22 0.14 0.24
EM1 0.16 0.17 1.83 1.28 1.3 1.8
kT2 [keV] 0.4 0.4 0.34 0.27 0.87 0.8 0.68
EM2 0.35 1.42 3.32 1.84 0.37 6.5
kT3 [keV] 1.0 1.0 0.75 0.81
EM3 0.01 1.1 2.71 0.65

kTwgt [keV] 0.33 0.63 0.44 0.31 0.545 0.29 0.58
reference Fuhrmeister et al. (2011) Fuhrmeister et al. (2011) Brown et al. (2023) Brown et al. (2023) Williams et al. (2014) Brown et al. (2023) Brown et al. (2023)

GJ 799A (quiescence) GJ 799A (flare) GJ144 GJ 820A GJ 820B GJ783A

SpT M4.5 K2 K5 K7 K2.5
distance [pc] 9.9 3.2 3.5 3.5 6.0

kT1 [keV] 0.2723 0.2508 0.12 0.21 0.19 0.17
EM1 2.34 2.71 53 4.09 1.71 5.31
kT2 [keV] 0.6696 0.7385 0.32 0.79 0.67 0.76
EM2 4.85 4.27 78.4 1.75 5.06 1.45
kT3 [keV] 1.982 2.9213 0.7
EM3 4.99 12.47 22.2
kTwgt [keV] 1.13 2.07 0.31 0.3838 0.55 0.30
reference Raassen et al. (2003) Raassen et al. (2003) Brown et al. (2023) Booth et al. (2017) Booth et al. (2017) Booth et al. (2017)

Notes. *EM is not listed in the paper. EM1 = EM2 = 0.5 is thus assumed for calculation.

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