Table D.2.
Spectral variability of the not simultaneous data between 3.0-10.0 keV.
| Name | Instrument | ObsID | Model | Γ | NH | Norm PL | Norm G | Flux | χ2/d.o.f |  |
Notes |
|---|---|---|---|---|---|---|---|---|---|---|---|
| (1022 cm−2) | (10−3) | (10−3) | (10−12 erg cm−2 s−1) | ||||||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) |
| NGC 4258* | XMM-Newton | 0400560301 | PL | # | # |  |
− | 3.84 |
- | - | We select |
| NuSTAR | 60101046004A | 1.61 |
7.67 |
 |
- | 2.18 |
443.2/387 | 1.145 | PL norm | ||
| 60101046004B | # | # | # | - | - | - | - | variable | |||
| ESO 253-G003* | XMM-Newton | 0762920501 | PL |  |
# | # | - | 0.45 |
- | - | Γ variable, |
| NuSTAR | 60101014002A |  |
2.29 |
0.19 |
- | 1.07 |
119.4/86 | 1.389 | We select only | ||
| 60101014002B | # | # | # | - | - | - | - | NuSTAR observations | |||
| NGC 3147* | XMM-Newton | 0405020601 | PL | # | # |  |
- | 1.14 |
- | - | We select |
| NuSTAR | 60101032002A | 1.79 |
2.98 |
 |
- | 2.19 |
243.5/217 | 1.122 | PL norm | ||
| 60101032002B | # | # | # | - | - | - | - | variable | |||
| NGC 2110* | XMM-Newton | 0145670101 | PL+G | # | # |  |
# | 25.00 |
- | - | We select |
| NuSTAR | 60061061004A | 1.53 |
3.84 |
 |
0.049 |
134.85 |
527.3/453 | 1.164 | PL norm | ||
| 60061061004B | # | # | # | # | - | - | - | variable | |||
| LEDA 96373* | XMM-Newton | 0674940101 | PL+G | # | # | 0.13 |
# | 1.14 |
- | - | We select PL norm tied, they |
| NuSTAR | 60061073002A | 0.93 |
13.59 |
0.17 |
0.022 |
1.40 |
245.2/141 | 1.739 | are consistent. The model | ||
| 60061073002B | # | # | # | # | - | - | - | is not enough to fit the data | |||
| NGC 2273* | XMM-Newton | 0140951001 | PL+G | # | # | 0.49 |
# | 0.93 |
- | - | We select |
| NuSTAR | 60001064002A | 1.56 |
30.04 |
0.53 |
0.037 |
0.98 |
109.7/102 | 1.075 | PL norm tied, they | ||
| 60001064002B | # | # | # | # | - | - | - | are consistent | |||
| NGC 7674* | XMM-Newton | 0200660101 | PL+G | # | # | 0.20 |
# | 0.052 |
- | - | Is a changing look, we |
| NuSTAR | 60001151002A | 1.71 |
18.28 |
0.49 |
0.0059 |
0.79 |
12.4/76 | 1.479 | did not combine the data. | ||
| 60001151002B | # | # | # | # | - | - | |||||
| IC 451A* | XMM-Newton | 0406410101 | PL+G | # | # |  |
# | 1.64 |
- | - | We select |
| NuSTAR | 60061260002A | 1.70 |
21.57 |
 |
0.015 |
4.29 |
143.4/123 | 1.166 | PL norm | ||
| 60061260002B | # | # | # | # | - | - | - | variable | |||
Notes: (Col. 1) name, (Col. 2) instrument, (Col. 3) obsID, (Col. 4) model, where "PL" represents the power-law and "G" a Gaussian component at 6.4 keV and σ=0.01 keV. (Col. 5) photon index, (Col. 6) column density, (Col. 7) Power-law normalization, (Col. 8) Normalization of the Gaussian component, (Col. 10 and 11) χ2/d.o.f., and 
, (Col. 12) Notes about the selection of the model. The case where the Normalization of the power-law (Norm PL) is a free parameter between the XMM-Newton and NuSTAR data is marked in boldface. The parameter in this table marked with # means that is tied to FPMA/NuSTAR. The symbol "−" denotes that these components were not required to improve the fit.
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