Table A.2.
Summary of best-fit solutions of Swift-XRT and NuSTAR data using different models for NGC 2788A
| Model | MyTorus | MyTorus | borus02 | |||||
|---|---|---|---|---|---|---|---|---|
| Edge-on | Face-on | |||||||
| C-Stat/dof | 136/153 | 116/153 | 116/151 | |||||
| CIns1a | 1.12 |
0.93 |
0.94 |
|||||
| CIns2b | 1.36 |
1.13 |
1.14 |
|||||
| Γ | 1.56 |
1.75 |
1.95 |
|||||
| CTor | — | — | 0.49 |
|||||
| θInc | — | — | 63 |
|||||
| NH,z | 3.95 |
1.95 |
2.34 |
|||||
| NH,S | 1.25 |
3.74 |
4.26 |
|||||
| fs 10−2 | 0.23 |
0.07 |
0.03 |
|||||
| F2 − 10keV | 4.36 |
4.56 |
4.50 |
|||||
| Fc10 − 50keV | 1.15 |
1.12 |
1.11 |
|||||
| L2 − 10keV | 9.48 |
5.33 |
11.29 |
|||||
| L10 − 50keV | 19.10 |
8.04 |
12.33 |
|||||
Notes. We summarise here the best-fits of joint Swift-XRT–NuSTAR spectra using different torus models at 0.8-50 keV, referred in Section 4.3. The statistics and degrees of freedom for each fit are also reported. The parameters are reported as in Table 2 if not mentioned otherwise.
CIns1 = CFPMA/XRT is the cross-calibration constant between NuSTAR observation of 2019 and Swift-XRT.
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