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Table 2.

Spectral fits parameters for the NuSTAR observations of 1ES 0229+200.

NuSTAR observation Model Normalization γ or α or Γ1 β or Γ2 Ebr χ2(d.o.f.)
(1) (2) (3) (4) (5) (6) (7)
nu21_02 PL 4.0 ± 0.2 2.32 ± 0.02 138(149)
LP 2.2 ± 0.4 1.7 ± 0.2 0.4 ± 0.1 135(148)
BKNPL 4.0 ± 0.2 2.32 ± 0.02 1.51 ± 0.02 26 ± 2 135(148)

nu21_04 PL 4.4 ± 0.3 2.40 ± 0.03 115(93)
LP 1.6 ± 0.4 1.3 ± 0.3 0.6 ± 0.1 100(92)
BKNPL 4.4 ± 0.3 2.41 ± 0.03 1.25 ± 0.02 26 ± 2 98(92)

nu21_06 PL 5.3 ± 0.3 2.37 ± 0.03 100(101)
LP 2.9 ± 0.6 1.7 ± 0.2 1.7 ± 0.2 96(100)
BKNPL 5.3 ± 0.3 2.37 ± 0.03 1.61 ± 0.03 25 ± 2 98(100)

nu13_02 PL 7.9 ± 0.5 2.02 ± 0.03 117(142)
LP 5.1 ± 1.1 1.6 ± 0.2 0.2 ± 0.1 111(141)

nu13_04 PL 8.8 ± 0.4 2.03 ± 0.02 228(193)
LP 5.7 ± 0.9 1.6 ± 0.2 0.2 ± 0.1 219( 192)

nu13_06 PL 7.7 ± 0.4 1.95 ± 0.02 174( 183)
LP 6.0 ± 1.0 1.7 ± 0.2 0.1 ± 0.1 171(182)

Notes. The following columns present (1) observation ID; (2) fitted model PL (single power-law), LP (logparabola), or BKNPL (broken power-law); (3) normalisation in 10−3 erg cm−2 s−1; (4) spectral parameter γ, α, or Γ1; (5) curvature parameter in the case of log-parabola model or second spectral index in the case of broken power-law model; (6) break energy of the broken power-law model; (7) χ2 and number of degrees of freedom for a model used.

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