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Table 3

Reduced χ2 values for the various time bins (f1 to f13), as marked in Fig. 3, for the different models of the photon spectrum (broken power-law (bknpo) and log parabola (logpar)) and the particle spectrum (cutoff power law, bknpo and log parabola), respectively.

State Obs id Photon spectrum Particle spectrum
XRT NuSTAR bknpo logpar CPL BPL LP

f1 00080050016 60002023024 1.27 1.02 1.07 1.06 1.03
f2 00032792001 60002023025 (a) 1.40 1.16 1.26 1.19 1.16
f3 60002023025 (b) 0.97 0.92 1.01 1.06 1.01
f4 00080050017 60002023025 (c) 1.22 1.04 1.08 1.07 1.05
f5 00080050018 60002023025 (d) 2.33 1.05 1.21 1.16 1.06
f6 00080050019 60002023027 2.93 1.08 1.41 1.39 1.09
f7 00032792002 60002023029 2.12 1.10 1.21 1.19 1.10
f8 00035014063 60002023031 2.45 1.14 1.20 1.31 1.13
f9 00035014064 60002023033 1.78 0.93 1.06 1.09 0.93
f10 00035014065 60002023035 1.75 1.10 1.09 1.10 1.10
f11 00035014066 60002023037 1.23 1.00 1.03 1.06 1.00
f12 00035014067 60002023039 1.14 1.01 1.08 1.02 1.01
f13 00035014068 1.07 1.07 1.04 1.07 0.92

Notes. Observation ids of XRT and NuSTAR are also given.

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