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Table 1.
Stars with no-detected magnetic field.
| Target | BD95% (G) | P3-σ |
|---|---|---|
| BN Ori | 2100 | 0 |
| CQ Tau | 1000 | 19 |
| HD 135127 | 4000 | 0 |
| HD 137059 | 400 | 82 |
| HD 143978 | 300 | 95 |
| IRAS 22152+6947 | 500 | 66 |
| NGC 2264 108 | 800 | 33 |
| NGC 2264 121 | 5200 | 0 |
| NGC 2264 84 | 450 | 84 |
| NGC 6530 SCB 739 | 70 | 100 |
| PAR 102 | 700 | 11 |
| PAR 1391 | 700 | 88 |
| PAR 1394 | 350 | 86 |
| PAR 1414 | 600 | 58 |
| PAR 1455 | 300 | 88 |
| PAR 1646 | 200 | 90 |
| PAR 1736 | 1500 | 5 |
| PAR 2441 | 180 | 100 |
| PX Vul | 1400 | 0 |
| RY Ori | 1000 | 62 |
Notes. Columns are: upper-limit of detection in the case of a dipolar field (BD95%, second row) and 3σ level probability of detecting complex, largescale magnetic field signatures of CV Cha-type (P3-σ, third row).
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