Table D.7.
Summary of the Cross normalization constants between the instruments.
| PEXMON | borus02 | XILLVER | |||||||
|---|---|---|---|---|---|---|---|---|---|
| Name | CA/B | CXMM | CBAT | CA/B | CXMM | CBAT | CA/B | CXMM | CBAT |
| NGC 3998 | 1.04 |
0.91 |
0.98 |
1.04 |
0.91 |
0.96 |
1.04 |
0.92 |
0.96 |
| NGC 3718 | 0.99 |
0.98 |
4.53 |
1.00 |
0.99 |
4.42 |
0.99 |
0.98 |
4.46 |
| NGC 4258* | 0.99 |
 |
2.64 |
0.99 |
 |
2.56 |
0.99 |
 |
2.60 |
| ESO 253-G003* | 1.14 |
- | 0.89 |
1.14 |
- | 0.88 |
1.14 |
- | 0.85 |
| NGC 1052 | 1.00 |
0.89 |
0.86 |
1.00 |
0.87 |
0.83 |
1.00 |
0.89 |
0.90 |
| NGC 2655 | 1.16 |
1.09 |
2.21 |
1.15 |
1.07 |
2.22 |
1.15 |
1.07 |
2.18 |
| NGC 3147* | 1.04 |
 |
1.08 |
1.04 |
0.99 |
1.00 |
1.04 |
0.92 |
1.08 |
| NGC 2110* | 1.03 |
 |
0.58 |
1.04 |
 |
0.60 |
1.03 |
 |
0.58 |
| LEDA 96373* | 1.12 |
0.84 |
0.87 |
1.13 |
0.87 |
0.85 |
1.12 |
0.86 |
0.88 |
| NGC 2992 | 1.027 |
0.91 |
0.127 |
1.026 |
0.909 |
0.122 |
1.026 |
0.915 |
0.13 |
| M 51 | 0.99 |
1.06 |
2.67 |
1.00 |
1.06 |
2.08 |
0.99 |
1.07 |
2.67 |
| NGC 2273* | 1.09 |
1.15 |
0.84 |
1.08 |
1.04 |
0.65 |
1.09 |
1.09 |
0.84 |
| HE 1136-2304 | 1.07 |
1.03 |
0.63 |
1.064 |
1.03 |
0.58 |
1.065 |
1.023 |
0.62 |
| IGRJ 11366-6002 | 1.15 |
- | 1.46 |
1.15 |
- | 1.42 |
1.15 |
- | 1.46 |
| IC 4518A* | 1.12 |
 |
1.11 |
1.11 |
 |
1.09 |
1.11 |
 |
1.09 |
| NGC 7674* | 1.02 |
- | 1.58 |
1.02 |
- | 1.60 |
1.02 |
- | 1.57 |
| NGC 5033 | 1.05 |
0.75 |
0.28 |
1.05 |
0.76 |
0.27 |
1.05 |
0.76 |
0.28 |
Notes: Name, cross normalization constant between the detector FPMA and FPMB of NuSTAR (CA/B, NuSTAR and XMM-Newton (CXMM) and NuSTAR and Swift (CBAT). In case of the not simultaneous data XMM-Newton+NuSTAR observations, where the normalization of the power-law is a free parameter (objects denoted in bold face), we put the restriction of CXMM=[0.9,1.10]. For IGRJ 11366-6002 we also obtain CXRT=1.30
(PEXMON), CXRT=1.13
(borus02) and CXRT=1.32
(XILLVER). The error of this parameters is in the normalization of the power-law then we reported here only the best fit value. The quantities in this table marked with ** are unconstrained errors.
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