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Table A.3.

Swift monitoring: Julian date, UT date, XRT 0.3–10 keV count rates (CR), and hardness ratios (HR(1)), X-ray photon index Γ, the observed 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).

Julian Date
2 400 000+ CR HR Γpl XRT flux (χ2/ν)pl
54266.6750 0.288 ± 0.008 +0.208 ± 0.024 1.88 ± 0.08 11.38 ± 0.26 39.8/50
54312.9792 0.215 ± 0.006 +0.178 ± 0.028 1.96 ± 0.08 8.29 ± 0.31 47.0/49
54361.9743 0.076 ± 0.003 +0.266 ± 0.033 1.78 ± 0.09 3.10 ± 0.14 48.7/42
54363.0389 0.079 ± 0.004 +0.386 ± 0.051 1.67 ± 0.14 3.51 ± 0.25 11.4/18
54364.1139 0.072 ± 0.003 +0.255 ± 0.044 1.89 ± 0.11 2.81 ± 0.09 25.9/23
54676.7875 0.268 ± 0.017 +0.311 ± 0.055 1.70 ± 0.17 11.45 ± 0.07 121/152 (2)
55092.9722 0.315 ± 0.005 +0.138 ± 0.015 2.04 ± 0.04 11.46 ± 0.02 216.0/163
56493.4166 0.067 ± 0.007 +0.305 ± 0.096 1.82 ± 0.29 2.91 ± 0.35 65.1/74 (2)
56556.3861 0.137 ± 0.017 +0.241 ± 0.127 1.92 ± 0.39 5.09 ± 0.92 49.5/50 (2)
57578.0396 0.048 ± 0.003 +0.345 ± 0.056 1.77 ± 0.16 2.10 ± 0.24 149.4/172 (2)
57856.3778 0.041 ± 0.009 +0.294 ± 0.159 1.78 ± 0.47 1.65 ± 0.33 27.7/33 (2)
57865.0097 0.035 ± 0.007 +0.057 ± 0.177 2.04 ± 0.62 1.35 ± 0.40 19.0/24 (2)
57880.7952 0.037 ± 0.007 +0.562 ± 0.136 2.30 ± 1.02 2.48 ± 0.16 18.4/26 (2)
57891.6903 0.035 ± 0.011 +0.383 ± 0.232 1.43 ± 0.42 (3)
57895.1028 0.033 ± 0.006 +0.554 ± 0.153 1.77 ± 0.58 1.41 ± 0.45 12.2/22 (2)
57896.0243 0.024 ± 0.006 −0.224 ± 0.241 2.25 ± 0.67 1.96 ± 0.34 16.8/16 (2)
57902.8451 0.018 ± 0.007 +0.348 ± 0.310 0.67 ± 0.27 (3)
57909.5556 0.017 ± 0.013 0.65 ± 0.50 (3)
57913.2708 0.026 ± 0.006 –0.002 ± 0.220 2.52 ± 0.66 1.30 ± 0.32 14.0/16 (2)
57916.4201 0.019 ± 0.004 +0.028 ± 0.200 2.01 ± 0.89 0.33 ± 0.12 15.2/28 (2)
57923.4986 0.016 ± 0.005 –0.211 ± 0.310 0.62 ± 0.29 (3)
57931.2806 0.014 ± 0.007 0.54 ± 0.27 (3)
57938.1931 0.017 ± 0.006 +0.056 ± 0.190 0.65 ± 0.23 (3)
57944.5639 0.020 ± 0.006 +0.435 ± 0.221 0.77 ± 0.23 (3)

Notes.

(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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