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Table 2.
Impact of our work on the number of DNe with known orbital periods.
| Group | Period range (d) | VSX | Table A.1 | Table A.2 | Total | Period range selection | |||
|---|---|---|---|---|---|---|---|---|---|
| N | N | % | N | % | N | % | |||
| A | 0.05–0.1 | 536 | 8 | 1.5 | 11 | 2.1 | 19 | 3.5 | Below the period gap |
| B | 0.1–0.13 | 15 | 0 | 0.0 | 1 | 6.7 | 1 | 6.7 | Within the gap |
| C | 0.13–0.42 | 227 | 16 | 7.0 | 51 | 22.5 | 67 | 29.5 | Above the gap, but < 10 h |
| D | 0.42–2.00 | 16 | 3 | 18.8 | 12 | 75.0 | 15 | 93.8 | > 10 h |
| Total | 0.05–2.00 | 794 | 27 | 3.4 | 75 | 9.4 | 102 | 12.8 | |
Notes. This table presents the increase in the total number (N) of DNe with known orbital periods as a result of the present study, along with approximate percentages reflecting our substantial contribution.
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