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Table 3.

Best fitting parameters used to fit the ISGRI flare data with the TBNEW × NTHCOMP model.

ID Date (MJD) Γ Te (keV) F20−200 (cgs) χ2/ν
F1 57382.51478 23.4/17
F2 57382.64095 15.3/17
F3 57382.66050 22.1/17
F4 57385.12628 14.0/17
F5 57385.25925 11.8/17
F6 57385.75382 14.3/17
F7 57385.86288 16.3/17
F8 57386.01908 14.3/17
F9 57386.26120 19.1/17
F10 57386.28652 6.6/17
F11 57386.29689 15.0/17
F12 57386.32638 7.1/17
F13 57386.61919 16.8/17
F14 57386.66460 16.8/17
F15 57386.67423 14.9/17
F16 57386.68682 19.6/17
F17 57386.92549 20.8/17
F18 57386.93660 16.9/17
F20 57386.98963 19.2/17
F21 57387.00889 23.9/17
F22a 57387.65443 8.9/16
F22b 57387.68924 18.6/16
F22c 57387.71063 19.6/16
F23a 57387.74620 8.5/16
F23b 57387.76239 22.0/16
F23c 57387.76894 17.9/16
F23d 57387.77413 9.0/16
F23e 57387.77635 13.7/16
F23f 57387.77931 19.3/16
F24a 57387.94133 19.8/17
F24b 57388.00629 13.4/16
F24c 57388.01147 14.6/16
F24d 57388.01369 12.9/16
F25 57388.02459 9.8/17
F26 57388.04829 12.1/17
F27 57388.33224 10.2/17
F28 57388.35505 18.5/17
F29 57388.43725 12.4/17
F30 57388.57621 22.6/17
F31 57388.60018 15.7/17
F32 57387.72808 13.9/17
F33 57388.73475 21.7/17
F34 57388.75840 11.0/17
F35a 57388.80567 12.7/16
F35b 57388.82343 21.0/17
F36 57388.86148 11.8/17
F37 57388.87037 15.6/17
F38 57388.88791 > 23 31.7/16
F39a 57388.91162 15.1/17
F39b 57388.96991 24.7/17

Notes. Time-resolved long ISGRI flares are separated with incrementing alphabets. The flare 19 (F19) was too faint to perform a meaningful spectral analysis. The fluxes are given in units of 10−8 erg cm−2 s−1. The seed photon temperature was fixed to 0.1 keV.

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