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Table 1

Characteristic quantities describing the parameter distributions (number of elements (#), mean (m), median (M), standard deviation (SD)), and best-fitting values from a Gaussian fit (mean (μ), standard deviation (σ)).

Name # μ σ m SD M

β op,X 65 0.95 ± 0.01 0.24 ± 0.02 1.03 0.50 0.95
β X 34 0.97 ± 0.02 0.18 ± 0.02 0.99 0.22 0.95
β op 34 0.47 ± 0.02 0.19 ± 0.02 0.48 0.20 0.48
log   (NH,BR/cm-2) 28 21.6 ± 0.11 0.51 ± 0.11 21.7 0.57 21.7
log   (NH,PL/cm-2) 43 21.7 ± 0.06 0.41 ± 0.06 21.9 0.48 21.7
E(B − V)MW 30 0.19 ± 0.02 0.14 ± 0.02 11.1 59.1 0.22
E(B − V)LMC 14 0.20 0.16 0.18
E(B − V)SMC 25 0.20 0.29 0.10
A V,MW 30 0.56 ± 0.10 0.42 ± 0.11 34.2 182. 0.69
A V,LMC 14 0.63 0.51 0.57
A V,SMC 25 0.59 0.87 0.29
log   (νrest,BR/Hz) 28 16.20 0.98 16.1

log   [(NH/cm-2)/(AV/mag)] MW 20 21.9 ± 0.05 0.04 ± 0.05 22.0 0.56 21.8
log   [(NH/cm-2)/(AV/mag)] LMC 12 22.6 ± 0.08 0.32 ± 0.11 22.4 0.95 22.6
log   [(NH/cm-2)/(AV/mag)] SMC 20 21.8 ± 0.16 0.87 ± 0.18 22.4 2.05 22.2

9 0.85 0.22 0.85
24 0.92 ± 0.03 0.21 ± 0.04 0.95 0.27 0.95
31 0.99 ± 0.03 0.23 ± 0.03 2.35 1.08 2.35
13 0.96 ± 0.02 0.10 ± 0.02 0.85 0.22 0.85
19 1.00 ± 0.08 0.29 ± 0.09 1.15 0.27 1.15
13 0.49 ± 0.04 0.14 ± 0.04 0.35 0.22 0.35
19 0.47 ± 0.08 0.29 ± 0.09 0.65 0.27 0.65
6 22.2 0.63 22.2
17 22.00 ± 0.14 0.67 ± 0.23 22.0 0.52 22.2
19 21.70 ± 0.04 0.30 ± 0.04 22.2 0.86 22.2
10 21.00 ± 1.20 0.93 ± 0.870 21.8 0.632 21.8
17 21.90 ± 0.05 0.23 ± 0.04 21.8 0.86 21.8
14 16.80 1.08 16.80
16 16.20 1.08 16.20

log   (LR,500 s/(erg s-1)) 64 45.90 ± 0.06 0.83 ± 0.06 46.00 3.72 45.90
log   (LR,1 h/(erg s-1)) 57 45.40 ± 0.06 0.73 ± 0.06 45.90 4.77 45.40
log   (LR,11 h/(erg s-1)) 40 44.50 ± 0.08 0.74 ± 0.08 45.70 7.44 44.50
log   (LR,1 day/(erg s-1)) 32 44.20 ± 0.11 0.83 ± 0.13 44.20 0.68 44.20

log   (FR,920 − 1200 s/(erg cm-2 s-1)) 46 –11.41 ± 0.07 0.34 ± 0.07 –11.31 0.80 –11.37
log   (F1 keV,920 − 1200 s/(erg cm-2 s-1)) 52 –12.54 ± 0.06 0.49 ± 0.06 –12.40 0.72 –12.45

Notes. The subscript PL indicates the values obtained by fitting the SED with a single power-law, while BR indicates a broken power-law. S stands for steep decay, P for plateau, and N for normal decay. The values of E(B − V) depend on the extinction model law used to fit the SED: Milky Way (MW), Large Magellanic Cloud (LMC) and Small Magellanic Cloud (SMC).

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