Table B.1.
NuSTAR orbit-wise analysis results of the four pointing on MJD 57757, MJD 57785, MJD 57813 and MJD 57840.
| MJD start | MJD end | F3−7 keV | F7−30 keV | α | β | χ2/dof |
|---|---|---|---|---|---|---|
| [10−10erg cm−2s−1] | [10−10erg cm−2s−1] | |||||
| 57757.0175 | 57757.0322 | 1.81 ± 0.02 | 1.81 ± 0.03 | 2.26 ± 0.09 | 0.11 ± 0.05 | 1.11 |
| 57757.0765 | 57757.0953 | 1.95 ± 0.02 | 2.07 ± 0.03 | 2.24 ± 0.09 | 0.10 ± 0.05 | 0.97 |
| 57757.1423 | 57757.1618 | 2.05 ± 0.02 | 2.23 ± 0.03 | 2.14 ± 0.08 | 0.15 ± 0.04 | 1.00 |
| 57757.2095 | 57757.2289 | 2.12 ± 0.02 | 2.21 ± 0.03 | 2.07 ± 0.07 | 0.21 ± 0.04 | 0.95 |
| 57757.2766 | 57757.2961 | 2.24 ± 0.02 | 2.35 ± 0.03 | 2.12 ± 0.07 | 0.19 ± 0.04 | 1.01 |
| 57757.3437 | 57757.3632 | 2.30 ± 0.02 | 2.30 ± 0.03 | 2.02 ± 0.08 | 0.26 ± 0.04 | 1.01 |
| 57757.4108 | 57757.4249 | 2.20 ± 0.02 | 2.17 ± 0.03 | 1.92 ± 0.09 | 0.31 ± 0.05 | 0.98 |
| 57757.4780 | 57757.4939 | 2.20 ± 0.02 | 2.20 ± 0.03 | 2.01 ± 0.08 | 0.26 ± 0.05 | 0.99 |
| 57785.0203 | 57785.0311 | 2.46 ± 0.02 | 2.74 ± 0.04 | 1.94 ± 0.08 | 0.24 ± 0.05 | 1.02 |
| 57785.0692 | 57785.0891 | 2.43 ± 0.02 | 2.63 ± 0.04 | 1.99 ± 0.09 | 0.23 ± 0.05 | 0.93 |
| 57785.1363 | 57785.1563 | 2.51 ± 0.03 | 2.81 ± 0.04 | 1.96 ± 0.09 | 0.23 ± 0.05 | 0.97 |
| 57785.2035 | 57785.2234 | 2.68 ± 0.03 | 2.96 ± 0.05 | 2.03 ± 0.10 | 0.20 ± 0.06 | 0.89 |
| 57785.2706 | 57785.2791 | 2.60 ± 0.03 | 2.92 ± 0.04 | 1.98 ± 0.09 | 0.21 ± 0.05 | 0.90 |
| 57785.3377 | 57785.3495 | 2.37 ± 0.02 | 2.37 ± 0.03 | 1.96 ± 0.09 | 0.29 ± 0.05 | 1.01 |
| 57785.4049 | 57785.4209 | 1.93 ± 0.02 | 1.76 ± 0.02 | 2.06 ± 0.09 | 0.28 ± 0.05 | 0.96 |
| 57785.4720 | 57785.4919 | 1.64 ± 0.01 | 1.49 ± 0.02 | 1.96 ± 0.09 | 0.35 ± 0.05 | 1.01 |
| 57785.5391 | 57785.5460 | 1.38 ± 0.02 | 1.08 ± 0.03 | 1.88 ± 0.17 | 0.47 ± 0.10 | 1.01 |
| 57812.9305 | 57812.9492 | 1.91 ± 0.02 | 1.71 ± 0.02 | 2.15 ± 0.08 | 0.24 ± 0.05 | 0.93 |
| 57812.9977 | 57813.0163 | 1.74 ± 0.02 | 1.58 ± 0.02 | 2.08 ± 0.09 | 0.27 ± 0.05 | 0.92 |
| 57813.0650 | 57813.0835 | 1.97 ± 0.02 | 1.92 ± 0.03 | 2.17 ± 0.08 | 0.18 ± 0.05 | 0.98 |
| 57813.1321 | 57813.1401 | 2.15 ± 0.03 | 2.20 ± 0.04 | 1.98 ± 0.11 | 0.26 ± 0.06 | 0.96 |
| 57813.1993 | 57813.2098 | 2.13 ± 0.02 | 2.13 ± 0.03 | 1.94 ± 0.10 | 0.30 ± 0.06 | 1.05 |
| 57813.2663 | 57813.2783 | 2.41 ± 0.02 | 2.44 ± 0.03 | 1.84 ± 0.09 | 0.35 ± 0.05 | 1.01 |
| 57813.3333 | 57813.3473 | 2.53 ± 0.02 | 2.49 ± 0.03 | 1.94 ± 0.08 | 0.30 ± 0.04 | 0.97 |
| 57813.4005 | 57813.4159 | 2.62 ± 0.02 | 2.58 ± 0.03 | 1.90 ± 0.07 | 0.34 ± 0.04 | 1.03 |
| 57813.4678 | 57813.4826 | 2.86 ± 0.02 | 2.92 ± 0.03 | 1.86 ± 0.07 | 0.33 ± 0.04 | 1.02 |
| 57839.9397 | 57839.9485 | 0.44 ± 0.01 | 0.28 ± 0.02 | 2.96 ± 0.34 | -0.03 ± 0.21 | 0.91 |
| 57839.9861 | 57840.0053 | 0.47 ± 0.01 | 0.33 ± 0.02 | 2.84 ± 0.37 | -0.05 ± 0.23 | 0.93 |
| 57840.0533 | 57840.0724 | 0.47 ± 0.01 | 0.36 ± 0.02 | 2.81 ± 0.29 | -0.04 ± 0.18 | 0.93 |
| 57840.1204 | 57840.1395 | 0.51 ± 0.01 | 0.40 ± 0.02 | 2.42 ± 0.24 | 0.18 ± 0.15 | 1.02 |
| 57840.1875 | 57840.2212 | 0.57 ± 0.01 | 0.50 ± 0.02 | 2.41 ± 0.20 | 0.11 ± 0.12 | 0.89 |
| 57840.2550 | 57840.2740 | 0.61 ± 0.01 | 0.47 ± 0.01 | 2.30 ± 0.18 | 0.23 ± 0.11 | 0.96 |
| 57840.3218 | 57840.3405 | 0.68 ± 0.01 | 0.54 ± 0.02 | 2.29 ± 0.17 | 0.22 ± 0.10 | 1.10 |
| 57840.3890 | 57840.4081 | 0.82 ± 0.01 | 0.72 ± 0.02 | 2.28 ± 0.15 | 0.17 ± 0.09 | 0.94 |
| 57840.4561 | 57840.4739 | 0.84 ± 0.01 | 0.71 ± 0.02 | 2.29 ± 0.13 | 0.20 ± 0.08 | 1.04 |
| 57840.5232 | 57840.5423 | 0.86 ± 0.01 | 0.72 ± 0.02 | 2.25 ± 0.13 | 0.23 ± 0.08 | 0.89 |
| 57840.5903 | 57840.6095 | 0.91 ± 0.01 | 0.74 ± 0.02 | 2.29 ± 0.13 | 0.21 ± 0.08 | 1.00 |
Notes. The start and end of the observations are listed in the first two columns. The second and third column are the 3-7 keV and 7-30 keV fluxes. The fifth and sixth column give the best-fit spectral parameters of the log-parabolic fits. The corresponding χ2/dof are listed in the last column.
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