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Table 2.

Results of the spectral fits using models tbabs × phabs × ∑2apec with temperatures fixed to kT1 = 0.75 keV and kT2 = 1.9 keV.

ID NH norm1 norm2 (d.o.f.)
(1022 cm−2) (10−3 cm−5) (10−3 cm−5) (10−12 erg cm−2 s−1)
0896/0200450201 0.52 ± 0.05 7.83 ± 0.56 3.90 ± 0.16 1.15 (226) 2.57 ± 0.04 7.23 2.26
0901/0200450301 0.44 ± 0.03 7.41 ± 0.34 4.16 ± 0.10 1.36 (397) 2.69 ± 0.03 8.02 2.33
0906/0200450401 0.48 ± 0.03 9.55 ± 0.35 4.49 ± 0.11 1.29 (416) 3.06 ± 0.03 9.23 2.63
0911/0200450501 0.50 ± 0.03 10.3 ± 0.44 2.82 ± 0.13 1.03 (307) 2.47 ± 0.04 8.91 2.00
1353/0505110301 0.72 ± 0.06 7.09 ± 0.51 2.30 ± 0.15 1.08 (224) 1.72 ± 0.04 4.39 1.48
1355/0505110401 0.70 ± 0.06 7.47 ± 0.51 2.54 ± 0.14 0.85 (221) 1.87 ± 0.03 4.81 1.61
2114/0677980601 0.71 ± 0.05 7.11 ± 0.44 1.74 ± 0.12 1.41 (108) 1.51 ± 0.04 4.31 1.25
2625/0740300101 0.39 ± 0.04 6.07 ± 0.41 3.22 ± 0.15 1.07 (251) 2.15 ± 0.04 7.07 1.84
3089/0780040101 0.55 ± 0.06 5.87 ± 0.46 2.52 ± 0.14 0.98 (181) 1.75 ± 0.04 4.96 1.52
3097/0793183001 0.58 ± 0.08 6.32 ± 0.78 4.30 ± 0.24 1.12 (107) 2.49 ± 0.07 5.70 2.76
3176/0800150101 0.48 ± 0.04 7.98 ± 0.44 3.20 ± 0.14 1.04 (299) 2.34 ± 0.04 7.59 1.98
3273/0801910201 0.30 ± 0.08 4.55 ± 0.72 4.52 ± 0.25 1.35 (103) 2.55 ± 0.07 7.31 2.30
3280/0801910301 0.51 ± 0.09 6.78 ± 0.95 3.84 ± 0.31 1.27 (87) 2.42 ± 0.08 6.46 2.15
3284/0801910401 0.21 ± 0.14 3.30 ± 1.05 4.63 ± 0.36 1.37 (71) 2.47 ± 0.10 6.98 2.27
3288/0801910501 0.28 ± 0.07 6.81 ± 0.89 4.47 ± 0.30 1.45 (101) 2.87 ± 0.08 10.1 2.49
3294/0801910601 0.48 ± 0.08 11.7 ± 1.3 3.69 ± 0.39 1.11 (83) 3.02 ± 0.11 10.6 2.51
00037920001 2.14 ± 0.74 16.2 ± 5.57 0.00 ± 0.93 0.50 (2) 1.12 ± 0.41 1.68 0.98
00031904001 0.39 ± 0.28 3.97 ± 2.24 3.99 ± 0.69 1.07 (23) 2.19 ± 0.20 5.49 2.01
00031904002 0.80 ± 0.32 7.10 ± 2.91 2.41 ± 0.74 1.25 (19) 1.72 ± 0.16 3.91 1.52
00031904003 0.47 ± 0.26 7.47 ± 2.93 3.75 ± 0.84 1.37 (25) 2.50 ± 0.22 7.42 2.18
00031904004 0.35 ± 0.32 4.10 ± 2.25 3.46 ± 0.64 0.61 (22) 2.01 ± 0.17 5.73 1.80
00031904005 1.26 ± 0.39 8.40 ± 3.40 2.13 ± 0.80 1.12 (15) 1.55 ± 0.19 2.44 1.42
00032767001 0.36 ± 0.64 1.40 ± 4.24 3.62 ± 1.45 1.01 (6) 1.69 ± 0.43 3.03 1.64
00032767002 0.77 ± 0.39 6.63 ± 3.47 1.98 ± 0.95 0.30 (11) 1.52 ± 0.18 3.77 1.32
00033818044 0.50 ± 0.71 8.50 ± 11.9 3.99 ± 3.75 1.86 (3) 2.71 ± 0.72 8.01 2.36
00032767003 0.94 ± 0.22 8.53 ± 2.17 2.74 ± 0.54 1.11 (37) 1.93 ± 0.13 3.85 1.73
00034282018 0.94 ± 0.57 9.30 ± 7.65 4.24 ± 2.19 0.81 (8) 2.57 ± 0.49 4.51 2.38
00093146005 0.44 ± 0.64 0.85 ± 3.20 4.79 ± 1.09 1.53 (8) 2.07 ± 0.50 2.73 2.06
00093148003 1.41 ± 0.73 7.91 ± 6.44 2.57 ± 1.63 1.42 (5) 1.60 ± 0.33 2.06 1.51
00034282086 0.88 ± 0.69 8.52 ± 9.39 3.35 ± 3.20 0.54 (4) 2.19 ± 0.68 4.32 1.98
00034282089 0.01 ± 0.87 1.40 ± 8.29 5.72 ± 2.39 0.17 (3) 2.81 ± 0.84 7.53 2.64
00010451001 1.05 ± 0.35 12.0 ± 5.12 4.77 ± 1.20 1.50 (18) 2.97 ± 0.20 4.88 2.75
00010451002 1.38 ± 0.71 6.22 ± 6.00 3.26 ± 1.33 0.61 (9) 1.69 ± 0.24 1.86 1.66
00010451003 1.42 ± 0.74 8.60 ± 5.50 1.30 ± 0.95 0.95 (8) 1.22 ± 0.19 1.93 1.09
00010451004 0.75 ± 0.42 5.27 ± 3.19 2.86 ± 0.79 1.28 (13) 1.71 ± 0.20 3.48 1.57
00010451005 0.85 ± 0.57 3.17 ± 3.19 3.92 ± 0.90 1.70 (14) 1.83 ± 0.23 2.39 1.80
00010451006 1.00 ± 0.32 9.67 ± 3.89 4.13 ± 0.98 1.02 (19) 2.53 ± 0.23 4.28 2.35
00010451007 1.00 ± 0.50 7.45 ± 4.91 4.42 ± 0.94 0.47 (18) 2.40 ± 0.22 3.58 2.29
00010451008 0.16 ± 0.54 1.08 ± 2.80 4.30 ± 0.76 1.29 (13) 2.02 ± 0.25 4.24 1.94
00010451009 0.52 ± 0.27 7.98 ± 3.13 3.29 ± 0.93 0.89 (18) 2.34 ± 0.23 7.04 2.02
00010451010 1.11 ± 0.45 11.4 ± 5.33 2.49 ± 1.13 0.81 (10) 2.04 ± 0.26 3.89 1.81
00094061006 0.92 ± 0.99 0.00 ± 3.95 3.32 ± 1.52 1.22 (1) 1.24 ± 1.31 0.83 1.30
00088806001 0.05 ± 0.67 3.14 ± 4.91 2.90 ± 1.33 1.64 (6) 1.80 ± 0.35 8.17 1.55
00088807001 0.20 ± 0.46 4.65 ± 4.58 3.00 ± 1.43 0.39 (6) 1.99 ± 0.34 8.06 1.69
2572 0.93 ± 0.14 7.52 ± 0.87 1.68 ± 0.14 1.33 (77) 1.43 ± 0.04 3.24 1.24
16659 0.59 ± 0.07 4.19 ± 0.28 2.77 ± 0.07 1.01 (722) 1.62 ± 0.02 3.67 1.48
402030010 0.44 ± 0.04 6.49 ± 0.43 4.14 ± 0.12 1.04 (1061) 2.55 ± 0.04 7.24 2.27

Notes. Unabsorbed fluxes are corrected for the interstellar column (2.04 × 1022 cm−2) only. Errors (found using the “error” command for the spectral parameters and the “flux err” command for the fluxes) correspond to 1σ; whenever errors were asymmetric, the largest value is provided here. Observed fluxes are expressed in the 0.5–10.0 keV band, while ISM-corrected fluxes are provided in the soft (0.5–2.0 keV) and hard (2.0–10.0 keV) bands. For each dataset, all available data were fit simultaneously: EPIC-pn, MOS1, and MOS2 for XMM-Newton, zeroth and first orders for Chandra, XIS-0, 1, and 3 for Suzaku.

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