Table 3.
Estimated unabsorbed luminosities in units of 1039 erg s−1 for each epoch using the distances from Table 1 and models from Table 2.
| Epoch | Lsoft | Lhard | Ltot | Lsoft diskbb | Lhard diskbb | Lsimpl |
|---|---|---|---|---|---|---|
| (0.3–1.5 keV) | (1.5–10 keV) | (0.3–10 keV) | (0.01–100 keV) | (0.01–100 keV) | (0.01–100 keV) | |
| Holmberg II X-1 | ||||||
| 1X | 6.1 ± 0.2 | 4.3 ± 0.1 | 10.4 ± 0.2 |
 |
 |
 |
| 2X | 5.5 ± 0.2 | 4.5 ± 0.2 | 10.0 ± 0.2 | 5. |
3.8 ± 0.9 | 8 ± 1 |
| 3X | 1.87 ± 0.05 | 0.57 ± 0.04 | 2.44 ± 0.06 | 2.4 ± 0.1 | 1.0 ± 0.1 | – |
| 4X | 6.56 ± 0.14 | 4.52 ± 0.06 | 11.1 ± 0.2 |
 |
 |
 |
| 5X |
 |
1.43 ± 0.03 |
 |
3.4 ± 0.1 | 1.79 |
 |
| 6XNN |
 |
4.23 ± 0.06 |
 |
4.7 ± 0.2 |
 |
 |
| 7XN |
 |
4.02 ± 0.06 | 8.0 ± 0.01 | 4.5 ± 0.2 |
 |
6.1 ± 0.3 |
Notes. For jointly fit data, the error estimation takes into account the errors on the joint parameters. Uncertainties are quoted at 90% confidence level. First column indicates the epoch given in Table 1 sorted chronologically. The simpl flux luminosity corresponds to the entire diskbb⊗simpl component. The full table is available at the CDS.
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