Table A.2.
Swift monitoring: MJD, XRT 0.3–10 keV count rates (CR), and hardness ratios (HR1), X-ray photon index Γ, the absorption corrected 0.3–10 keV X-ray flux in units of 10−12 erg s−1 cm−2, and reduced χ2 of the simple power-law model fit (pl) with Galactic Absorption.
MJD | CR | HR1 | Γpl | XRT Flux | (χ2/ν)pl |
---|---|---|---|---|---|
54266.1750 | 0.286±0.011 | +0.208±0.024 | 1.88±0.08 | 11.40±0.42 | 39.8/52 |
54312.4792 | 0.238±0.008 | +0.178±0.028 | 1.96±0.08 | 8.30±0.31 | 47.0/49 |
54361.4743 | 0.083±0.003 | +0.266±0.033 | 1.78±0.09 | 3.10±0.14 | 48.7/42 |
54362.5389 | 0.086±0.004 | +0.386±0.051 | 1.67±0.14 | 3.52±0.24 | 11.4/18 |
54363.6139 | 0.079±0.003 | +0.255±0.044 | 1.89±0.11 | 2.81±0.09 | 25.9/25 |
54676.2875 | 0.288±0.020 | +0.311±0.055 | 1.70±0.17 | 11.45±0.76 | 167/1542 |
55092.4722 | 0.340±0.007 | +0.138±0.015 | 2.04±0.04 | 11.46±0.02 | 216.0/1632 |
56492.4166 | 0.073±0.008 | +0.305±0.096 | 1.82±0.29 | 2.91±0.35 | 65.1/742 |
56555.8861 | 0.149±0.018 | +0.241±0.127 | 1.92±0.39 | 5.09±0.92 | 49.5/502 |
57577.5396 | 0.051±0.003 | +0.345±0.056 | 1.77±0.16 | 2.10±0.24 | 149.4/1722 |
57855.7061 | 0.037±0.009 | +0.212±0.240 | 1.78±0.47 | 1.65±0.33 | 27.7/332 |
57855.8778 | 0.045±0.010 | +0.367±0.210 | —- | 1.11±0.303 | — |
57864.5097 | 0.045±0.010 | +0.057±0.177 | 2.04±0.62 | 1.35±0.40 | 19.0/242 |
57880.2952 | 0.040±0.008 | +0.562±0.136 | 2.30±1.02 | 2.48±0.16 | 18.4/262 |
57891.1903 | 0.029±0.010 | +0.383±0.232 | — | 1.43±0.423 | — |
57894.6028 | 0.032±0.008 | +0.554±0.153 | 1.77±0.58 | 1.41±0.45 | 12.2/222 |
57895.0243 | 0.024±0.006 | -0.224±0.241 | 2.25±0.67 | 1.96±0.34 | 16.8/162 |
57902.3451 | 0.018±0.007 | +0.348±0.310 | — | 0.67±0.273 | — |
57909.0556 | 0.017±0.013 | —- | — | 0.65±0.503 | — |
57912.7708 | 0.030±0.007 | -0.002±0.220 | 2.52±0.66 | 1.30±0.32 | 14.0/162 |
57915.9201 | 0.018±0.004 | +0.028±0.200 | 2.01±0.89 | 0.33±0.12 | 15.2/282 |
57922.9986 | 0.016±0.005 | -0.211±0.310 | — | 0.62±0.293 | — |
57930.7806 | 0.014±0.007 | —- | — | 0.54±0.273 | — |
57937.6931 | 0.021±0.006 | +0.056±0.190 | — | 0.65±0.233 | — |
57944.0639 | 0.022±0.006 | +0.435±0.221 | — | 0.77±0.233 | — |
58705.4279 | 0.403±0.033 | +0.137±0.074 | 1.87±0.16 | 11.77±0.66 | 116/1512 |
58740.6404 | 0.200±0.018 | +0.133±0.079 | 1.92±0.23 | 6.59±0.84 | 87.6/912 |
58746.2726 | 0.355±0.042 | +0.073±0.053 | 2.07±0.22 | 10.60±1.10 | 70.7/1012 |
58759.5462 | 0.298±0.030 | +0.219±0.073 | 1.84±0.17 | 10.04±0.88 | 167/1432 |
58761.9466 | 0.400±0.048 | +0.186±0.083 | 2.01±0.21 | 13.89±1.30 | 104/1012 |
58769.3119 | 0.161±0.014 | +0.160±0.058 | 1.98±0.25 | 3.95±0.50 | 74.0/792 |
58769.4993 | 0.179±0.014 | +0.000±0.190 | 1.71±0.20 | 7.55±0.57 | 116/1222 |
58770.7026 | 0.148±0.013 | +0.056±0.094 | 2.05±0.25 | 3.37±0.48 | 75.0/742 |
58779.6649 | 0.303±0.028 | +0.257±0.093 | 1.95±0.23 | 9.28±1.15 | 117/812 |
58782.0028 | 0.337±0.049 | +0.355±0.135 | 1.50±0.47 | 16.86±4.71 | 32.5/382 |
58792.7181 | 0.265±0.016 | +0.095±0.064 | 1.91±0.14 | 8.26±0.43 | 191/1802 |
58793.4931 | 0.266±0.016 | +0.108±0.099 | 1.78±0.24 | 15.13±1.95 | 96.2/802 |
58796.5980 | 0.306±0.022 | +0.198±0.049 | 1.91±0.23 | 9.28±1.25 | 117/832 |
58804.5670 | 0.154±0.015 | +0.091±0.076 | 1.98±0.25 | 4.91±0.70 | 75.2/842 |
58823.3669 | 0.127±0.015 | +0.062±0.125 | 1.90±0.31 | 3.57±0.49 | 28.9/582 |
58830.8669 | 0.152±0.014 | +0.362±0.081 | 1.69±0.22 | 5.22±0.42 | 79.3/912 |
58837.5791 | 0.291±0.033 | +0.070±0.087 | 1.90±0.23 | 8.70±0.71 | 72.4/882 |
58851.0457 | 0.233±0.018 | +0.247±0.072 | 1.69±0.17 | 8.49±0.82 | 98.6/1442 |
58858.2817 | 0.308±0.023 | +0.168±0.071 | 1.93±0.17 | 7.81±0.73 | 119/1332 |
59312.1285 | 0.085±0.013 | +0.121±0.150 | 1.95±0.40 | 2.69±0.40 | 36.0/362 |
59313.2613 | 0.138±0.014 | +0.341±0.088 | 1.63±0.25 | 5.11±0.61 | 54.8/792 |
1 The hardness ratio is defined as HR = , where soft and hard are the background-corrected counts in the 0.3–1.0 keV and 1.0–10.0 keV bands, respectively
2 Fit using Cash statistics (Cash 1979)
3 Extrapolated from the XRT count rates using the flux and count rate of the MJD 57865 observation
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