Table D.6.
Summary of other parameters of the best fit models.
| PEXMON | borus02 | XILLVER | ||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Name | NH, W | log(ξW) | Norm PLXMM | Norm PLNu | NH, W | log(ξW) | Norm PLXMM | Norm PLNu | NH, W | log(ξW) | Norm PLXMM | Norm PLNu |
| (1022 cm−2) | (10−3) | (10−3) | (1022 cm−2) | (10−3) | (10−3) | (1022 cm−2) | (10−3) | (10−3) | ||||
| NGC 3998 | - | - | # | 2.33 |
- | - | # | 2.35 |
- | - | # | 2.05 |
| NGC 3718 | - | - | # | 0.53 |
- | - | # | 0.52 |
- | - | # | 0.08 |
| NGC 4258* | - | - | 1.70 |
1.13 |
- | - | 1.60 |
1.04 |
- | - | 0.032 |
0.021 |
| ESO 253-G003* | - | - | - | 0.17 |
- | - | - | 0.30 |
- | - | - | 0.02 |
| NGC 1052 | 0.05 |
6 |
# | 2.79 |
- | - | # | 3.46 |
19.25 |
2.032 |
# | 0.043 |
| NGC 2655 | 2.11 |
1.32 |
# | 0.91 |
- | - | # | 0.80 |
2.57 |
1.36 |
# | 0.02 |
| NGC 3147* | - | - | 1.89 |
0.68 |
- | - | 0.34 |
0.71 |
- | - | 0.0066 |
0.012 |
| NGC 2110*w | 0.17 |
-0.55 |
10.80 |
59.40 |
1.53 |
4.30 |
8.38 |
4.44 |
5.23 |
1.36 |
0.30 |
1.54 |
| LEDA 96373* | 0.79 |
-0.93 |
# | 0.12 |
0.80 |
-0.55 |
# | 5.93 |
7.94 |
2.01 |
# | 0.005 |
| NGC 2992 | 0.49 |
2.53 |
# | 18.58 |
0.64 |
2.48 |
# | 20.80 |
- | - | # | 0.40 |
| M 51 | 499.96 |
4.25 |
# | 0.056 |
- | - | # | 0.36 |
488.99 |
4.18 |
# | 0.0012 |
| NGC 2273* | 2.95 |
1.24 |
# | 0.29 |
0.94 |
-1.14 |
# | 5.14 |
2.97 |
1.23 |
# | 0.006 |
| HE 1136-2304 | - | - | # | 2.53 |
- | - | # | 2.53 |
- | - | # | 0.0042 |
| IGRJ 11366-6002 | - | - | - | 2.42 |
- | - | - | 2.26 |
- | - | - | 1.43 |
| IC 4518A* | 3.79 |
1.37 |
0.77 |
1.65 |
4.41 |
1.44 |
0.65 |
2.13 |
3.97 |
1.39 |
0.015 |
0.032 |
| NGC 7674* | - | - | - | 0.36 |
- | - | - | 0.24 |
- | - | - | 0.003 |
| NGC 5033 | - | - | # | 1.93 |
- | - | # | 1.90 |
- | - | # | 0.032 |
Notes: Name, Column density and ionization degree of the warm absorber (NH, W and log(ξW)) and the normalization of the power law emission of XMM-Newton and NuSTAR observations (Norm PLXMM and Norm PLNu). The parameter in this table marked with # (power-law normalization of XMM-Newton) is tied to NuSTAR, "−" denotes that these were not required to improve the fit. Objects with * symbols are galaxies with no simultaneous observations. NGC 2110 (denoted as NGC 2110w) need two warm absorbers to improve the pexmon fit. In addition to the absorber presented in this table, the other correspond to: NH, W=5.38
and log(ξW)=1.31
.
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