Table 1
Derived orbital solutions.
| Object | T 0 | P | γ | K | e norm | log pfalse [10%] | log pfalse [1%] |
| [HJD−2 450 000] | [d] | [km s-1] | [km s-1] | [km s-1] | |||
|
|
|||||||
| HE 1415−0309 | 5240.909 ± 0.002 | 0.192 ± 0.004 | 104.7 ± 9.5 | 152.4 ± 11.2 | 18.6 | −1.0 | −0.4 |
| HS 2359+1942 | 6279.221 ± 0.007 | 0.93261 ± 0.00005 | −96.1 ± 6.0 | 107.4 ± 6.8 | 8.3 | −1.2 | −1.1 |
| LB 1516 | 5495.73 ± 0.05 | 10.3598 ± 0.0005 | 14.3 ± 1.1 | 48.6 ± 1.4 | 4.4 | < −4.0 | < −4.0 |
|
|
|||||||
| BPS CS 22879−149 | 5413.102 | 0.478 | 21.9 ± 2.5 | 63.5 ± 2.8 | 5.4 | ... | ... |
| 5412.448 | 0.964 | −25.5 ± 5.3 | 121.7 ± 6.3 | 6.2 | ... | ... | |
|
|
|||||||
| OGLE BUL−SC16 335 | 4758.614 | 0.122 | 36.4 ± 19.6 | 92.5 ± 26.2 | 25.1 | ... | ... |
| HS 2043+0615 | 4254.610 ± 0.003 | 0.3015 ± 0.0003 | −43.5 ± 3.4 | 73.7 ± 4.3 | 8.3 | ... | ... |
| PG 0941+280 | 4476.185 | 0.311 | 73.0 ± 4.9 | 141.7 ± 6.3 | 19.4 | ... | ... |
| V 1405 Ori | 4477.362 | 0.398 | −33.6 ± 5.5 | 85.1 ± 8.6 | 15.2 | ... | ... |
|
|
|||||||
Notes. The systematic error adopted to normalise the reduced χ2 (enorm) is given for each case. The probabilities for the orbital period to deviate from our best solution by more than 10% (pfalse [10%]) or 1% (pfalse [1%]) are given in the last columns. The last four lines show the binaries, where the orbital period has been determined from photometry.
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