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Table 1.
Percentage of subhalos detected (predicted to be in the correct or adjacent mass bin) across the test set with apparent source magnitudes between [17−21].
| 108 M⊙ | 108.5 M⊙ | 109 M⊙ | 109.5 M⊙ | 1010 M⊙ | |
|---|---|---|---|---|---|
| 50 HST Orbits, simple lens | 0.8 | 17.1 | 58.9 | 87.9 | 97.1 |
| 1 HST Orbit, simple lens | 0.0 | 3.3 | 22.1 | 55.5 | 80.2 |
| 50 HST Orbits, complicated lens | 2.0 | 22.1 | 59.3 | 86.7 | 96.9 |
| 1 HST Orbit, complicated lens | 0 | 2.8 | 16.6 | 45.3 | 73.9 |
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