Table 3
Measured and predicted flux in spectral regions where 56Ni lines are expected to be as a function of models.
| Model | Energy band | Measured flux | Predicted flux | Probability |
| (keV) | (10-4 photons s-1 cm-2) | (10-4 photons s-1 cm-2) | % | |
|
|
||||
| DETO | 150–175 | –0.20 ± 0.78 | 0.81 | 92.4 |
| 265–295 | –0.55 ± 0.85 | 0.48 | ||
| 482–508 | 0.13 ± 0.88 | 0.36 | ||
| 730–880 | –1.01 ± 2.02 | 2.01 | ||
|
|
||||
| SCOP3D | 145–170 | –0.50 ± 0.76 | 0.70 | 84.7 |
| 267–297 | –0.24 ± 0.86 | 0.36 | ||
| 482–508 | 0.13 ± 0.88 | 0.27 | ||
| 720–880 | –0.75 ± 2.08 | 1.54 | ||
|
|
||||
| SC3F | 150–170 | –0.03 ± 0.67 | 0.37 | 62.4 |
| 253–283 | –0.99 ± 0.85 | 0.25 | ||
| 452–508 | 0.38 ± 1.42 | 0.29 | ||
| 720–880 | –0.75 ± 2.08 | 0.76 | ||
|
|
||||
| SC1F | 150–170 | –0.03 ± 0.67 | 0.32 | 51.8 |
| 254–288 | –0.81 ± 0.90 | 0.22 | ||
| 458–509 | 0.01 ± 1.37 | 0.23 | ||
| 725–900 | –1.02 ± 2.18 | 0.63 | ||
|
|
||||
| HED6 | 159–169 | –0.13 ± 0.49 | 0.08 | 21.3 |
| 270–284 | –0.98 ± 0.59 | 0.05 | ||
| 475–505 | –0.27 ± 1.04 | 0.06 | ||
| 746–872 | –0.13 ± 1.87 | 0.27 | ||
|
|
||||
| DDTc | 158–165 | –0.10 ± 0.57 | 0.03 | 6.2 |
| 270–282 | –0.58 ± 0.76 | 0.02 | ||
| 480–498 | –1.22 ± 1.00 | 0.02 | ||
| 740–880 | 1.28 ± 2.08 | 0.08 | ||
|
|
||||
| W7 | 158–165 | –0.34 ± 0.69 | 0.02 | 3.4 |
| 270–282 | –0.88 ± 0.92 | 0.02 | ||
| 478–498 | –1.82 ± 1.37 | 0.02 | ||
| 740–880 | –0.31 ± 1.38 | 0.04 | ||
|
|
||||
| DDTe | 158–165 | –0.34 ± 0.69 | 0.01 | 2.0 |
| 270–280 | –0.49 ± 0.84 | 0.008 | ||
| 480–498 | –1.00 ± 1.26 | 0.009 | ||
| 740–880 | –0.152 ± 3.25 | 0.05 | ||
Notes. The fifth column is the probability of rejecting the model (see text). In the case of DDTc, W7 and DDTe models, the fluxes were obtained for an optimal observation periods of 7, 5 and 5 days, respectively (see Table 4).
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