Table 4
Best-fit parameters of the Cen X-3 Obs ID 30101055002 pulse and amplitude models compared to spectral results (Tomar et al. 2021).
| PF | 1st | 2nd | Spectral | ||
|---|---|---|---|---|---|
 |
2.0/10 | 2.0/8 | 0.8/17 | – | |
 |
1.1/29 | 1.6/27 | 0.8/23 | – | |
 |
3 | 2 | 2 | – | |
 |
2 | 7 | 2 | – | |
| Esplit | 10.71 | 9.40 | 13.82 | – | keV |
| AFe | −0.060 ± 0.003 | −0.0241 ± 0.0018 | −0.0265 ± 0.0016 |  |
|
| EFe | 6.485 ± 0.018 | 6.43 ± 0.02 | 6.55 ± 0.03 | 6.67(a) | keV |
| σFe | 0.56 ± 0.02 | 0.47 ± 0.03 | 0.57 ± 0.03 | 0.53(a) ± 0.03 | keV |
| ACyc | −1.14 ± 0.13 |  |
 |
0.40 ± 0.13 | |
| ECyc | 29.5 ± 0.3 | 27 ± 3 | 29.1 ± 0.3 | 30.3 ± 0.6 | keV |
| σCyc | 3.8 ± 0.3 |  |
 |
5.0 ± 0.9 | keV |
Notes. 
and 
are the reduced χ2 for the lower- and higher-energy sections, respectively, with 
and 
the corresponding polynomial orders. Esplit is the energy at which we separate the two regions. (a)Tomar et al. (2021) model the iron line with a complex of three lines at 6.4, 6.67, and 6.97 keV. Here we report the width of the central one, which is fitted to the data and representative of the full width.
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