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Table 1.
Summary.
| Star type | South | North | Total |
|---|---|---|---|
| Original sample | 1014 | 492 | 1506 |
| ssrAp candidates | 60 | 67 | 127 |
| Resolved magnetically split lines | 19 | 8 | 27 |
| Sharp unresolved lines | 10 | 7 | 17 |
| v sin i ≲ 20 km s−1 | 0 | 3 | 3 |
| Broad lines/v sin i > 20 km s−1 | 6 | 0 | 6 |
| Accurate rotation period values | 6 | 14 | 20 |
| Prot > 50 d | 6 | 11 | 17 |
| 26 d < Prot < 50 d | 0 | 3 | 3 |
| Prot < 26 d? | 0 | 3 | 3 |
| Stars with magnetic field measurements | 24 | 17 | 41 |
| Definite roAp stars | 12 | 5 | 17 |
| Possible roAp stars | 1 | 8 | 9 |
| Fraction of roAp stars | 22% | ≲19% | ≲20% |
| Definite δ Sct stars | 2 | 9 | 11 |
| Possible δ Sct stars | 1 | 5 | 6 |
| Possible eclipsing binaries | 1 | 2 | 3 |
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