Table 4.
Run-test on the fit residuals of the broad emission Fe K line of the NS LMXB GX 13+1.
| Obs. | Energy | Run-test (a) (%) |  (χ2/d.o.f.) |
||||
|---|---|---|---|---|---|---|---|
| (keV) | Gaussian | Windline | Diskline | Gaussian | Windline | Diskline | |
| 1 | 6.0–6.67 | 12.6 | 20.0 | 14.4 | 1.16 (1714.58/1480) | 1.21 (1784.81/1481) | 1.14 (1690.81/1478) |
| 2 | 6.0–6.67 | 55.2 | 56.9 | 43.0 (b) | 1.06 (1578.99/1486) | 1.06 (1572.35/1485) | 1.06 (1573.37/1483) (b) |
| 2 | 6.0–6.67 | 32.4 (c) | 1.07 (1588.06/1483) (c) | ||||
Notes.
Probability that n consecutive data points in the emission line region are mutually independent.
Value corresponding to the fit in which the emission line energy is not constrained (see Col. 7 Table 3).
Value corresponding to the fit in which the emission line is constrained in the 6.4–6.97 keV energy range (see Col. 8 Table 3).
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