Table A.1
Details of the HST data used in this paper.
| VFTS | HST ID | Filter | Integration time |
| [s] | |||
|
|
|||
| 089 | APPP-LMC | F814W | 3200 |
| 123 | 9741 | F814W | 3200 |
| 208 | 9741 | F814W | 2800 |
| 216 | 9741 | F814W | 2800 |
| 382 | 8163 | F814W | 85 |
| 385 | 8163 | F814W | 85 |
| 392 | 8163 | F814W | 85 |
| 398 | 8163 | F814W | 85 |
| 470 | 8163 | F814W | 85 |
| 488 | 8163 | F814W | 85 |
| 537 | 8163 | F814W | 85 |
| 577 | 8163 | F814W | 85 |
| 581 | 8163 | F814W | 85 |
| 682 | 8163 | F673N | 2000 |
| 706 | 5114 | F814W | 1200 |
| 849 | APPP-SFD | F606W | 1760 |
Notes. The completeness limit tests that we conducted were done on VFTS 385, which is amongst the shortest exposure times. This means that our completeness limit of 2 to 3 M⊙ is a worst-case scenario. The HST ID column refers to the proposal IDs when available, otherwise they refer to the APPP repository (Wadadekar et al. 2006).
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