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Table 5.
Spectral fits of the p0 interval with the hot*pion2*pion1*(bb+comt) model.
| Interval | p0 |
|---|---|
| Parameter | |
| hot | |
| NHcold (1022 cm−2) | 6.0 ± 0.1 |
| blackbody | |
| kTbb (keV) | 1.23 ± 0.01 |
| Norm (1013 cm2) | 1.0 ± 0.5 |
| comt | |
| kTbb (keV) | (c) |
| kThot (keV) | 2.91 ± 0.04 |
| τ | 10 (f) |
| Norm (1044 ph s−1 keV−1) | 24 ± 2 |
| pion1 | |
| NHpion (1022 cm−2) | 5 ± 2 |
| log ξ (erg cm s−1) | 4 (f) |
| σv (km s−1) | 50 (f) |
| v (km s−1) | −307 ± 44 |
| Solid angle | 0.16 ± 0.07 |
| pion2 | |
| NHpion2 (1022 cm−2) | 17 ± 4 |
| log ξ (erg cm s−1) | 3.51 ± 0.06 |
| σv (km s−1) | 51 ± 10 |
| v (km s−1) | −139 ± 15 |
| Covering fraction | 0.60 ± 0.09 |
Lumin |
5.8 × 1037 |
| C-stat. (d.o.f.) | 3200 (2921) |
| Cross-normalization NuSTAR FPMA | 0.98 |
| Cross-normalization NuSTAR FPMB | 0.98 |
Notes. For each interval, we fitted the 2−10 keV XRISM and 4−30 keV NuSTAR spectra simultaneously. f indicates a fixed parameter and c a coupled parameter. The cross-normalisation for NuSTAR with respect to Resolve is indicated in the last rows.
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