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Table 2.
Best-fit χ2 of the different models in Class 5 and their comparison.
| Source | Source | Coupled MYTorus | Decoupled MYTorus | ϵ (%) | Fixed Γ | F-test | Model |
|---|---|---|---|---|---|---|---|
| name | id | χ2/d.o.f. | χ2/d.o.f. | χ2/d.o.f. | Pnull (%) | ||
| IGR J00254+6822 | 64 | 48.9/42 | 43.9/41 | 30.8 | 56.9/43 | 1.2 | CMwF |
| IGR J02501+5440 | 65 | 9.7/21 | 8.1/20 | 39.9 | 9.7/22 | 100.0 | CMwF |
| SWIFT J0453.4+0404 | 66 | 889.4/774 | 774.9/773 | 4 × 10−23 | 795.2 / 774 | 8 × 10−4 | DM |
| SWIFT J0601.9–8636 | 67 | 62.9/44 | 64.5/43 | 12.1 | 106.9 / 45 | 2 × 10−4 | CM |
| SWIFT J1009.3–4250 | 68 | 104.7/106 | 94.6/105 | 2.0 | 106.9/107 | 13.9 | CMwF |
| IGR J13091+1137 | 69 | 277.9/231 | 263.4/230 | 0.2 | 277.9/231 | 0.05 | DM |
| IGR J14175–4641 | 70 | 61.2/54 | 47.8/53 | 0.4 | 48.3/54 | 46.0 | DMwF |
| IGR J16351–5806 | 71 | 78.3/71 | 73.6/70 | 31.8 | 78.7/72 | 54.9 | CMwF |
| IGR J20286+2544 | 72 | 55.9/61 | 52.3/60 | 55.9 | 55.9/62 | 100.0 | CMwF |
| LEDA 15023 | 73 | 122.9/95 | 116.5/94 | 12.4 | 128.7/96 | 3.7 | CMwF |
| LEDA 96373 | 74 | 118.5/100 | 104.3/99 | 0.3 | 110.4/100 | 1.8 | DMwF |
| MCG –03-34-064 | 75 | 783.2/567 | 643.5/566 | 10−28 | 713.7/567 | 2 × 10−12 | DM |
| Mrk 3 | 76 | 5222.4/2207 | 2574.4/2206 | 0.0 | 2757.4/2207 | 8 × 10−33 | DM |
| NGC 1194 | 77 | 114.0/124 | 110.7/123 | 58.6 | 154.9/125 | 8 × 10−8 | CM |
| NGC 3281 | 78 | 181.0/204 | 178.1/203 | 67.1 | 218.3/205 | 7 × 10−8 | CM |
| NGC 4507 | 79 | 2549.3/1674 | 1864.4/1673 | 5 × 10−147 | 1940.7/1674 | 3 × 10−14 | DM |
| NGC 4941 | 80 | 46.2/35 | 43.8/34 | 84.2 | 48.5/36 | 19.5 | CMwF |
| NGC 5643 | 81 | 126.5/111 | 127.9/110 | 15.8 | 286.1/112 | 2 × 10−19 | CM |
| NGC 5728 | 82 | 270.6/279 | 259.5/278 | 1.0 | 284.0/280 | 0.02 | CM |
| NGC 788 | 83 | 114.8/123 | 96.3/122 | 2.9 ⋅ 10−2 | 99.1/123 | 6.2 | DMwF |
Notes. The last column lists the model used for each source: coupled MYtorus (CM), decoupled MYtorus (DM), coupled MYtorus with fixed slope (CMwF), and decoupled MYtorus with fixed slope (DMwF).
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