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Table 3

Spectral fitting results.

Region Excess counts(1) Γ/kT(2) Surface flux(3) (d.o.f.)

M 62
Ring0 660.1 ± 43.3 8.9 ± 0.3 2.51 ± 0.42 1.2(504)
Ring1 897.4 ± 49.5 9.6 ± 0.1 2.18 ± 0.26
Ring2 1145.9 ± 48.1 9.8 ± 0.1 2.05 ± 0.20
Ring3 1175.2 ± 50.8 9.9 ± 0.1 1.82 ± 0.12
Ring4 1669.7 ± 58.3 9.6 ± 0.2 2.22 ± 0.19
Ring5 1750.0 ± 78.7 9.7 ± 0.1 2.18 ± 0.18
Ring6 850.1 ± 41.8 9.0 ± 0.4 1.91 ± 0.15
Ring7 223.9 ± 14.8 8.6 ± 0.5 2.18 ± 0.25
Ring8 326.5 ± 17.7 9.0 ± 0.6 2.13 ± 0.20
Outer 1672.5 ± 74.8 0.40 ± 0.03 5.74 ± 0.37 1.3(99)

NGC 6388
Ring0 264.9 ± 26.5 5.6 ± 1.2 6.65 ± 2.4 1.1(469)
Ring1 318.0 ± 37.8 6.8 ± 1.1 3.79 ± 1.3
Ring2 392.2 ± 38.1 7.0 ± 0.9 3.34 ± 0.91
Ring3 446.8 ± 37.0 6.6 ± 0.9 3.72 ± 0.98
Ring4 457.6 ± 29.6 7.1 ± 0.9 2.63 ± 0.66
Ring5 580.4 ± 46.2 6.9 ± 0.9 3.03 ± 0.71
Ring6 681.4 ± 46.6 7.4 ± 0.9 2.76 ± 0.61
Ring7 705.5 ± 55.4 7.1 ± 0.8 3.20 ± 0.64
Ring8 657.7 ± 45.6 7.3 ± 0.9 2.58 ± 0.59
Outer 1966.9 ± 76.5 0.18 ± 0.02 8.25 ± 0.55 1.1(88)

NGC 6541
Ring0 442.5 ± 47.3 8.9 ± 0.3 1.56 ± 0.19 1.4(451)
Ring1 730.2 ± 53.8 9.2 ± 0.2 1.42 ± 0.13
Ring2 917.3 ± 63.4 9.5 ± 0.1 1.34 ± 0.10
Ring3 769.7 ± 58.8 9.2 ± 0.2 1.39 ± 0.12
Ring4 437.4 ± 21.0 9.5 ± 0.1 1.20 ± 0.09
Ring5 547.5 ± 23.1 9.1 ± 0.1 1.47 ± 0.10
Ring6 450.1 ± 21.6 9.2 ± 0.2 1.38 ± 0.11
Ring7 367.1 ± 20.0 9.4 ± 0.2 1.25 ± 0.11
Ring8 345.0 ± 18.9 9.4 ± 0.2 1.25 ± 0.11
Outer 1767.8 ± 81.0 0.17 ± 0.02 5.51 ± 0.39 0.9(67)

M 80
Ring0 187.6 ± 24.6 2.5 ± 1.6 10.8 ± 8.0 1.4(567)
Ring1 210.6 ± 28.5 2.6 ± 1.4 6.9 ± 5.7
Ring2 291.6 ± 28.4 3.3 ± 0.6 3.1 ± 1.5
Ring3 360.6 ± 32.2 3.2 ± 0.5 3.9 ± 1.7
Ring4 432.2 ± 35.1 1.6 ± 0.9 16 ± 11
Ring5 538.8 ± 42.5 2.2 ± 0.5 8.1 ± 3.6
Ring6 626.3 ± 43.2 2.0 ± 0.6 10 ± 5.0
Ring7 673.4 ± 51.3 2.5 ± 0.4 6.0 ± 2.2
Ring8 711.8 ± 45.5 2.2 ± 0.4 9.4 ± 3.4
Outer 2309.4 ± 79.0 0.42 ± 0.08 26.0 ± 2.5 1.2(182)

Notes. The quoted uncertainties are 90% confidence intervals calculated by letting each free parameter vary. Therefore, parameter correlations are taken into account. (1) Total number of excess counts summed over all contributing CCDs in the energy bands 1–7 keV (Ring1–8) and 0.7–10.0 keV (Outer). (2) This column gives the photon index in the cases where an absorbed powerlaw spectrum was fitted (Ring1–8), or kT in units of keV for the combined Outer region. (3) Observed surface flux in units of 10-8 erg cm-2 s-1 sr-1 in the energy bands 1–7 keV (Ring1–8) and 0.7–10.0 keV (Outer).

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