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Table A.2.

Example of the Swift-XRT results for 1ES 1959+650.

(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)
Date OBS ID Exp. ΓPL χ2/d.o.f. ΓLP βLP χ2/d.o.f. Prob.( ⋆ ) F2 − 10 keV F0.3 − 10 keV
(MJD) (s) (%) (×10−11 erg cm−2s−1)
56572.10 00035025108 1064 2.08 ± 0.03 0.45 ± 0.06 307.8/233 10−4 11.8 ± 0.4 25.9 ± 0.4
56779.02 00035025109 1041 2.04 ± 0.05 0.49 ± 0.10 107.4/117 10−3 4.3 ± 0.2 9.3 ± 0.2
56786.88 00035025110 648 2.33 ± 0.04 84.6/70 1.00 3.6 ± 0.3 7.9 ± 0.3
56793.73 00035025111 754 2.16 ± 0.06 0.50 ± 0.14 76.1/80 0.02 3.1 ± 0.3 7.5 ± 0.3
56807.95 00035025112 962 2.19 ± 0.05 0.39 ± 0.11 59.8/87 10−3 2.9 ± 0.2 6.8 ± 0.2
56821.13 00035025114 993 2.10 ± 0.05 77.0/58 3.21 6.3 ± 0.4 11.6 ± 0.4
56842.19 00035025116 994 2.08 ± 0.03 133.3/132 2.65 7.9 ± 0.3 14.2 ± 0.3
56848.52 00035025117 910 2.06 ± 0.05 0.43 ± 0.12 96.3/82 0.08 4.3 ± 0.3 9.2 ± 0.3
56856.67 00035025118 1260 2.05 ± 0.03 0.46 ± 0.07 182.8/174 10−4 5.4 ± 0.3 11.6 ± 0.3
56863.53 00035025119 885 2.01 ± 0.03 0.38 ± 0.07 166.8/164 10−3 7.7 ± 0.3 15.6 ± 0.3

Notes. Columns: (1) Observation date. (2) Observation ID. (3) Exposure time. (4) Spectral index of the PL model. (5) χ2/d.o.f. of the fitted PL model. (6) Spectral index of the LP model. (7) Curvature parameter of the fitted LP model. (8) χ2/d.o.f. of the LP model. (9) Null-hypotheses probability of the F-test. (10) X-ray flux in the range of 2–10 keV. (11) X-ray flux in the range of 0.3–10 keV.

( ⋆ )The LP model is preferred over the PL model at 3σ confidence level if the F-test probability value is less than 0.27%. Only the first ten lines of the table are shown. Data are available for all five targets at the CDS.

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