Table A.1
Best fit parameters for all the sources.
| hot | pow | comt | bb | dbb | xabs | |||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| obsID | NH | Γ | kBT | τ | kBT | kBT | NH | logξ | v | F0.5−2 keV | F2−10 keV | Cstat/d.o.f |
| (1022 cm−2) | (kev) | (kev) | (kev) | (1020 cm−2) | (102 km s−1) | (10−10 erg cm−2 s−1) | (10−9 erg cm−2 s−1) | |||||
| GRS 1758-258 | ||||||||||||
| 2429 | 2.14 ± 0.05 | 3.9 ± 0.2 | – | – | 0.90 ± 0.06 | – | – | – | – | 0.79 ± 0.08 | 0.12 ± 0.01 | 12621∕11561 |
| 2750 | 2.8 ± 0.1 | – | – | 1.00 ± 0.01 | – | – | – | – | 1.2 ± 0.2 | 0.42 ± 0.06 | ||
| GRS 1915+105 | ||||||||||||
| 660 | 5.06 ± 0.02 | – | – | – | – | 3.0 ± 0.1 | 3 ± 1 | 2.7 ± 0.2 | − 7 ± 2 | 1.5 ± 0.1 | 7.8 ± 0.8 | 6056∕5241 |
| 7485 | – | – | – | – | 12 ± 3 | 5.9 ± 0.7 | 3.72 ± 0.02 | − 1.45 ± 0.09 | 1.3 ± 0.4 | 23 ± 7 | ||
| GX 3+1 | ||||||||||||
| 16492 | 1.91 ± 0.05 | 1.12 ± 0.04 | – | – | 0.8 ± 0.1 | – | – | – | – | 3.7 ± 0.2 | 7.5 ± 0.5 | 28199/27207 |
| 16307 | 1.09 ± 0.04 | – | – | 0.8 ± 0.1 | – | – | – | – | 3.6 ± 0.2 | 7.4 ± 0.5 | ||
| 18615 | 1.25 ± 0.04 | – | – | 0.7 ± 0.2 | – | – | – | – | 2.6 ± 0.1 | 4.8 ± 0.3 | ||
| 19890 | 1.23 ± 0.03 | – | – | 0.8 ± 0.2 | – | – | – | – | 3.3 ± 0.2 | 6.1 ± 0.4 | ||
| 19907 | 1.21 ± 0.04 | – | – | 0.7 ± 0.1 | – | – | – | – | 2.7 ± 0.1 | 4.8 ± 0.3 | ||
| 19957 | 1.20 ± 0.03 | – | – | 0.8 ± 0.2 | – | – | – | – | 3.4 ± 0.2 | 6.9 ± 0.4 | ||
| 19958 | 1.22 ± 0.03 | – | – | 0.8 ± 0.1 | – | – | – | – | 3.3 ± 0.2 | 6.2 ± 0.4 | ||
| GX 9+1 | ||||||||||||
| 11088 | 1.65 ± 0.02 | – | 2.4 ± 0.4 | 22 ± 9 | 0.76 ± 0.04 | – | – | – | – | 0.53 ± 0.04 | 10 ± 1 | 4815∕4293 |
| GX 17+2 | ||||||||||||
| 717 | 2.19 ± 0.01 | – | 2.5 ± 0.1 | 16 ± 4 | 0.79 ± 0.02 | – | – | – | – | 4.3 ± 0.2 | 13 ± 1 | 4946/4244 |
| H 17433-322 | ||||||||||||
| 16738 | 2.67 ± 0.09 | 1.47 ± 0.04 | – | – | – | 0.38 ± 0.09 | – | – | – | 0.35 ± 0.02 | 0.88 ± 0.05 | 19169∕18365 |
| 17679 | 1.47 ± 0.03 | – | – | – | 0.45 ± 0.05 | – | – | – | 0.21 ± 0.01 | 0.54 ± 0.03 | ||
| 17680 | 1.48 ± 0.04 | – | – | – | 0.42 ± 0.06 | – | – | – | 0.35 ± 0.02 | 0.91 ± 0.05 | ||
| 16739 | 1.49 ± 0.04 | – | – | – | 0.44 ± 0.08 | – | – | – | 0.39 ± 0.02 | 0.96 ± 0.05 | ||
| IGR J17091-3624 | ||||||||||||
| 12406 | 1.20 ± 0.01 | 1.78 ± 0.03 | – | – | 0.86 ± 0.01 | – | – | – | – | 2.5 ± 0.1 | 1.9 ± 0.1 | 17403∕16586 |
| 17787 | 2.04 ± 0.02 | – | – | 0.55 ± 0.01 | – | – | – | – | 2.3 ± 0.2 | 1.1 ± 0.1 | ||
| 17788 | 1.99 ± 0.03 | – | – | 0.69 ± 0.01 | – | – | – | – | 1.9 ± 0.1 | 1.0 ± 0.1 | ||
| LMC X-1 | ||||||||||||
| 93 | 0.79 ± 0.01 | 2.46 ± 0.03 | – | – | 0.61 ± 0.01 | – | – | – | – | 1.6 ± 0.1 | 0.38 ± 0.03 | 22659∕21818 |
| 11074 | 2.45 ± 0.04 | – | – | 0.63 ± 0.01 | – | – | – | – | 1.7 ± 0.1 | 0.42 ± 0.04 | ||
| 11986 | 2.65 ± 0.05 | – | – | 0.68 ± 0.01 | – | – | – | – | 1.4 ± 0.1 | 0.32 ± 0.03 | ||
| 11987 | 2.44 ± 0.04 | – | – | 0.62 ± 0.01 | – | – | – | – | 1.6 ± 0.1 | 0.37 ± 0.03 | ||
| 12068 | 2.40 ± 0.03 | – | – | 0.70 ± 0.01 | – | – | – | – | 1.7 ± 0.1 | 0.47 ± 0.04 | ||
| 12071 | 2.59 ± 0.05 | – | – | 0.61 ± 0.01 | – | – | – | – | 1.8 ± 0.1 | 0.39 ± 0.04 | ||
| 12069 | 2.51 ± 0.07 | – | – | 0.64 ± 0.01 | – | – | – | – | 1.7 ± 0.1 | 0.41 ± 0.03 | ||
| 12070 | 2.62 ± 0.06 | – | – | 0.60 ± 0.01 | – | – | – | – | 1.6 ± 0.1 | 0.34 ± 0.03 | ||
| 12089 | 2.58 ± 0.05 | – | – | 0.64 ± 0.01 | – | – | – | – | 1.6 ± 0.1 | 0.35 ± 0.03 | ||
| 12090 | 2.79 ± 0.06 | – | – | 0.67 ± 0.01 | – | – | – | – | 1.6 ± 0.1 | 0.34 ± 0.03 | ||
| 12072 | 2.59 ± 0.03 | – | – | 0.72 ± 0.01 | – | – | – | – | 1.5 ± 0.1 | 0.37 ± 0.03 | ||
Notes. We report the parameter values for each model used in the analysis where kB T indicates the temperature, NH the column density, Γ the photon index of the power-law model, ξ the ionisation parameter, v the flow velocity (which, in the case of a negative number, corresponds to the outflow velocity), and F0.5−2 keV and F2−10 keV the fluxes in the two different energy ranges. Errors given on parameters are 1σ errors. We also list the obsID of each observation and the C-statistic and degree of freedom (dof) for every fit.
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