Table D.3.
Baseline plus sine function best-fitting parameters for the re-binned 0.2-1 keV EPIC-pn light curves from the XMM12 observation.
| QPE type | Trec | C | N | σ | A | P |
|---|---|---|---|---|---|---|
| QPE(w) | 20.05 ± 0.05 | 0.359 ± 0.007 | 0.54 ± 0.03 | 743 ± 48 | 0.098 ± 0.007 | 54 ± 4 |
| QPE(s) | − | 1.87 ± 0.05 | 913 ± 21 | − | − |
Notes. The first five columns are the same as in Table D.2. The additional sine function has normalisation A (in units of cts s−1) and period P (in units ks). The best-fitting baseline plus sine function models results in χ2/ν = 140/46. Removing the sine function from the fit produces χ2/ν = 550/49. We use a time-bin of 1 000 s.
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