Table 3.
Spectral fitting of the NuSTAR blazars.
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
---|---|---|---|---|---|---|---|
Source | Obs. ID | Model | Γ, Γ1 | Eb(keV) | β, Γ2 | ![]() |
F-value (prob.) |
S5 0014+81 | 60001098002 | PL | 1.82 ± 0.03 | – | – | 1.1851/153 | |
LP | 1.84 ± 0.04 | – | 0.36 ± 0.12 | 1.1226/152 | 9.52 (2.42 × 10−3) | ||
BPL | 1.73 ± 0.04 | 21.79 ± 2.56 | 3.40 ± 0.73 | 1.0706/151 | 9.18 (1.73 × 10−4) | ||
60001098004 | PL | 1.70 ± 0.03 | – | – | 1.1128/164 | ||
LP | 1.70 ± 0.03 | – | 0.00 ± 0.11 | 1.1197/163 | – | ||
BPL | 1.71 ± 0.04 | 19.55 ± 16.11 | 1.56 ± 0.28 | 1.1231/162 | 0.25 (7.81 × 10−1) | ||
B0222+185 | 60001101002 | PL | 1.54 ± 0.02 | – | – | 0.9783/479 | |
LP | 1.54 ± 0.02 | – | 0.22 ± 0.05 | 0.9380/478 | 21.58 (4.39 × 10−6) | ||
BPL | 1.47 ± 0.03 | 14.04 ± 2.09 | 1.75 ± 0.07 | 0.9405/477 | 10.63 (3.06 × 10−5) | ||
60001101004 | PL | 1.64 ± 0.02 | – | – | 0.9882/366 | ||
LP | 1.66 ± 0.02 | – | 0.29 ± 0.06 | 0.9270/365 | 25.16 (8.24 × 10−7) | ||
BPL | 1.34 ± 0.08 | 6.54 ± 0.70 | 1.75 ± 0.03 | 0.9149/364 | 15.66 (2.99 × 10−7) | ||
HB 0836+710 | 60002045002 | PL | 1.69 ± 0.02 | – | – | 0.9106/452 | |
LP | 1.69 ± 0.02 | – | –0.08 ± 0.05 | 0.9075/451 | 2.54 (1.11 × 10−1) | ||
BPL | 1.73 ± 0.03 | 12.65 ± 4.07 | 1.60 ± 0.06 | 0.9045/450 | 2.52 (8.13 × 10−2) | ||
60002045004 | PL | 1.66 ± 0.01 | – | – | 1.0267/664 | ||
LP | 1.66 ± 0.01 | – | 0.10 ± 0.04 | 1.0146/663 | 8.92 (2.93 × 10−3) | ||
BPL | 1.59 ± 0.03 | 7.98 ± 1.83 | 1.70 ± 0.03 | 1.0156/662 | 4.63 (1.01 × 10−2) | ||
3C 273 | 10202020002 | PL | 1.62 ± 0.00 | – | – | 1.0871/1335 | |
LP | 1.62 ± 0.00 | – | 0.11 ± 0.01 | 1.0326/1334 | 71.46 (7.31 × 10−17) | ||
BPL | 1.57 ± 0.01 | 13.43 ± 1.05 | 1.72 ± 0.02 | 1.0299/1333 | 38.07 (8.32 × 10−17) | ||
10302020002 | PL | 1.66 ± 0.01 | – | – | 0.9334/1017 | ||
LP | 1.66 ± 0.01 | – | 0.08 ± 0.02 | 0.9164/1016 | 19.87 (9.23 × 10−6) | ||
BPL | 1.64 ± 0.01 | 19.35 ± 3.23 | 1.78 ± 0.05 | 0.9190/1015 | 8.97 (1.38 × 10−4) | ||
3C 279 | 60002020002 | PL | 1.73 ± 0.02 | – | – | 0.9442/480 | |
LP | 1.73 ± 0.02 | – | 0.08 ± 0.05 | 0.9411/479 | 2.58 (1.09 × 10−1) | ||
BPL | 1.71 ± 0.02 | 29.87 ± 8.06 | 2.15 ± 0.33 | 0.9386/478 | 2.43 (8.90 × 10−2) | ||
60002020004 | PL | 1.74 ± 0.01 | – | – | 0.9031/691 | ||
LP | 1.74 ± 0.01 | – | 0.07 ± 0.03 | 0.8982/690 | 4.77 (2.93 × 10−2) | ||
BPL | 1.69 ± 0.03 | 8.66 ± 2.40 | 1.78 ± 0.03 | 0.8980/689 | 2.96 (5.24 × 10−2) | ||
PKS 1441+25 | 90101004002 | PL | 2.08 ± 0.08 | – | – | 1.030/49 | |
LP | 2.01 ± 0.09 | – | –0.32 ± 0.28 | 1.027/48 | 1.14 (2.90 × 10−1) | ||
BPL | 2.09 ± 0.09 | 23.56 ± 23.32 | 1.51 ± 1.38 | 1.070/47 | 0.08 (9.19 × 10−1) | ||
PKS 2149–306 | 60001099002 | PL | 1.37 ± 0.01 | – | – | 0.9722/824 | |
LP | 1.36 ± 0.01 | – | 0.05 ± 0.03 | 0.9686/823 | 4.06 (4.42 × 10−2) | ||
BPL | 1.34 ± 0.02 | 12.48 ± 3.57 | 1.42 ± 0.03 | 0.9668/822 | 3.30 (3.73 × 10−2) | ||
60001099004 | PL | 1.46 ± 0.01 | – | – | 0.9730/744 | ||
LP | 1.46 ± 0.01 | – | 0.04 ± 0.03 | 0.9716/743 | 2.07 (1.50 × 10−1) | ||
BPL | 1.42 ± 0.03 | 8.86 ± 2.94 | 1.49 ± 0.02 | 0.9701/742 | 2.11 (1.22 × 10−1) | ||
1ES 0229+200 | 60002047004 | PL | 2.03 ± 0.02 | – | – | 1.0547/387 | |
LP | 2.06 ± 0.02 | – | 0.23 ± 0.07 | 1.0255/386 | 12.02 (5.86 × 10−4) | ||
BPL | 1.99 ± 0.03 | 16.04 ± 3.42 | 2.30 ± 0.15 | 1.0390/385 | 3.92 (2.06 × 10−2) | ||
S5 0716+714 | 90002003002 | PL | 1.90 ± 0.03 | – | – | 1.2050/194 | |
LP | 1.87 ± 0.03 | – | –0.33 ± 0.09 | 1.1428/193 | 11.56 (8.19 × 10−4) | ||
BPL | 1.94 ± 0.04 | 19.60 ± 5.08 | 1.50 ± 0.23 | 1.1922/192 | 2.04 (1.33 × 10−1) | ||
Mrk 501 | 60002024002 | PL | 2.27 ± 0.01 | – | – | 0.8889/562 | |
LP | 2.30 ± 0.02 | – | 0.16 ± 0.04 | 0.8649/561 | 16.59 (5.29 × 10−5) | ||
BPL | 2.26 ± 0.01 | 19.77 ± 5.55 | 2.48 ± 0.16 | 0.8848/560 | 2.30 (1.01 × 10−1) | ||
60002024004 | PL | 2.24 ± 0.01 | – | – | 1.0918/730 | ||
LP | 2.26 ± 0.01 | – | 0.13 ± 0.03 | 1.0650/729 | 19.37 (1.24 × 10−5) | ||
BPL | 2.23 ± 0.01 | 24.50 ± 4.37 | 2.55 ± 0.14 | 1.0786/728 | 5.47 (4.40 × 10−3) |
Notes. Column 1: source name, Col. 2: Obs. ID, Col. 3: spectral models, power-law (PL), log-parabola (LP), broken power-law (BPL), Col. 4: photon index (PL and LP), high-energy photon index (BPL), Col. 5: break energy (keV), Col. 6: Curvature Parameter (LP), low-energy photon index (BPL), Col. 7: reduced χ2/degrees of freedom, and Col. 8: F-test and probability value. The best-fit spectral models are given in bold font.
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