Table 4.
Number of new early-type candidates.
| Method | All | m < 16 | R < 14″ | m < 16 & R < 14″ |
|---|---|---|---|---|
| MLP | 498 | 229 | 351 | 148 |
| XGBoost | 311 | 141 | 294 | 124 |
| Bayesian | 204 | 134 | 185 | 116 |
| Common | 155 | 98 | 145 | 88 |
Notes. We defined a candidate early-type star as one with an unknown spectral type and a probability of being early larger than 0.5. The Common row includes the early-type candidates identified consistently by all three methods. The magnitudes m are extinction-corrected IB224 magnitudes after the local calibration (see Section 3.3.2). R is the projected distance from Sgr A*.
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