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Table B.1.

Best-fit values of the seven data sets 955, 2735, 2736, 2737, 2738, 15747, 16527 with the power law model.

(1) (2) (3) (4) (5) (6) (7) (8)
Obs. N H 47 Tuc + local $ N_{\mathrm{H}}^{\mathrm{47 Tuc + local}} $ Γ Fabs χ red 2 $ \chi^2_{\rm red} $ (d.o.f.)a n.h.p.b Γ Fabs
(1021 cm−2) (10−14 erg cm−2 s−1) (10−14 erg cm−2 s−1)



955 2.0 2.0 + 14.2 $ ^{+14.2}_{-2.0} $ 1.3 0.5 + 1.1 $ ^{+1.1}_{-0.5} $ 8 ± 4 0.18(2) 0.84 1.3 0.4 + 0.5 $ ^{+0.5}_{-0.4} $ 7 2 + 4 $ ^{+4}_{-2} $
2735 1.7 1.7 + 2.2 $ ^{+2.2}_{-1.7} $ 1.4 0.2 + 0.3 $ ^{+0.3}_{-0.2} $ 7 ±1 1.03(15) 0.42 1.5 ± 0.2 6.4 0.8 + 1.2 $ ^{+1.2}_{-0.8} $
2736 4.0 2.9 + 3.7 $ ^{+3.7}_{-2.9} $ 1.6 ± 0.3 6 ± 1 1.31(14) 0.19 1.5 ± 0.2 6.2 0.8 + 1.0 $ ^{+1.0}_{-0.8} $
2737 3.8 2.2 + 2.6 $ ^{+2.6}_{-2.2} $ 1.5 0.2 + 0.3 $ ^{+0.3}_{-0.2} $ 8 ± 1 2.02(18) 0.01 1.4 ± 0.2 8 ± 1
2738 2.7 2.3 + 2.5 $ ^{+2.5}_{-2.3} $ 1.8 ± 0.3 7 ± 1 0.93(18) 0.54 1.75 ± 0.2 7.0 0.8 + 1.2 $ ^{+1.2}_{-0.8} $
15747 2.9 (frozen) 1.7 ± 0.3 5 ± 1 0.47(7) 0.86 1.65 ± 0.3 5.1 0.8 + 1.1 $ ^{+1.1}_{-0.8} $
16527 2.9 (frozen) 1.3 0.4 + 0.5 $ ^{+0.5}_{-0.4} $ 4 1 + 2 $ ^{+2}_{-1} $ 2.33(3) 0.07 1.3 0.4 + 0.5 $ ^{+0.5}_{-0.4} $ 4 1 + 2 $ ^{+2}_{-1} $

Notes. The fit was performed assuming N H GAL = 5.5 × 10 20 $ N_{\mathrm{H}}^{\mathrm{GAL}} = 5.5 \times 10^{20} $ cm−2 and for two different cases: independent fits for each spectrum (columns 2–6) and simultaneous fit with the same local absorption (columns 7–8). The latter fit resulted in N H 47 Tuc + local = ( 2 . 6 1.1 + 1.2 ) × 10 21 $ N_{\mathrm{H}}^{\mathrm{47 Tuc + local}}=(2.6^{+1.2}_{-1.1})\times 10^{21} $ cm−2, with χ red 2 $ \chi^2_{\rm red} $(d.o.f.) = 1.22(81) and n.h.p. = 0.08. Fluxes are computed in the energy range 0.5–6 keV. (a)Degrees of freedom (d.o.f). (b)Null hypothesis probability (n.h.p.).

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