Table 2.
Models falling within all observational uncertainties.
| Model | Md0 [M⊙] | MBH0 [M⊙] | Porb0[d] | β | tobs [Myr] | χ2(tobs) | |χred2−1| |
|---|---|---|---|---|---|---|---|
| A | 1.4 | 9.0 | 0.65 | 0.5 | 6352 | 1.34 | 0.73 |
| B | 1.25 | 8.5 | 0.80 | 0.5 | 8027 | 1.04 | 0.79 |
| C | 1.25 | 9.1 | 0.82 | 0.5 | 7115 | 1.03 | 0.79 |
| D | 1.1 | 8.6 | 1.16 | 0.5 | 9991 | 0.98 | 0.80 |
| E | 1.1 | 8.8 | 1.16 | 1.0 | 10 053 | 0.94 | 0.81 |
| F | 1.4 | 8.9 | 0.65 | 0.5 | 6295 | 0.39 | 0.92 |
Notes. From left to right, the columns include the model name, initial masses for the donor star and BH, initial orbital period, β parameter value, the age at which the system best falls within the observational errors, the χ2 statistic value at that moment, and the distance from the unit of the reduced chi-square (χ2/ν, where ν are the degrees of freedom).
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