Table 3
Her X-1 ObsID 30002006005.
| PF | 1st | 2nd | Spectral | ||
|---|---|---|---|---|---|
 |
0.7/10 | 0.5/10 | 1.5/14 | –– | |
 |
1.0/47 | 1.2/47 | 1.2/45 | –– | |
 |
4 | 4 | 3 | –– | |
 |
3 | 3 | 2 | –– | |
| Esplit | 11.17 | 11.01 | 12.82 | –– | keV |
| AFe | −0.072 ± 0.002 | −0.0486 ± 0.0016 |  |
(6.3 ± 0.7) × 10−3 | |
| EFe | 6.503 ± 0.008 | 6.524 ± 0.008 | 6.51 ± 0.05 | 6.55 ± 0.05 | keV |
| σFe | 0.418 ± 0.010 | 0.422 ± 0.010 |  |
 |
keV |
| ACyc | −10.4 ± 0.7 | −6.9 ± 0.5 | −2.36 ± 0.09 | 0.6 ± 0.3 | |
| ECyc | 40.44 ± 0.15 | 40.32 ± 0.16 | 40 10 ± 0 16 | 37.4 ± 0.2 | keV |
| σCyc | 6.82 ± 0.19 | 7.2 ± 0.2 | 5.18 ± 0.14 | 5.8 ± 0.3 | keV |
Notes. Comparison of best-fit parameters for the fundamental amplitude, second harmonic amplitude, and for the PF computed by averaging over all the fitted harmonic amplitudes. Spectral fit results from Fürst et al. (2013) using a power law with a high-energy cutoff. 
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.
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