Table 1
Metrics describing the performance of our halo star classifier for the three different cases depending on the training features available.
Ideal GUMS sample with G < 12.5 mag | |||
---|---|---|---|
6D phase-space + phot +[Fe/H] | 6D phase-space + phot | 5D phase-space + phot | |
recall | 0.94 | 0.90 | 0.84 |
precision | 0.99 | 0.98 | 0.98 |
logarithmic loss | 0.01 | 0.01 | 0.01 |
Matthews coef | 0.96 | 0.94 | 0.90 |
GUMS sample with G < 12.5 mag convolved with median TGAS uncertainties | |||
6D phase-space + phot +[Fe/H] | 6D phase-space + phot | 5D phase-space + phot | |
recall | 0.71 | 0.64 | 0.46 |
precision | 0.90 | 0.87 | 0.82 |
logarithmic loss | 0.01 | 0.01 | 0.01 |
Matthews coef | 0.80 | 0.75 | 0.62 |
Error convolved GUMS sample with Gaia DR2 uncertainties | |||
6D phase-space + phot +[Fe/H]a | 6D phase-space + phota | 5D phase-space + photb | |
recall | 0.93 | 0.90 | 0.58 |
precision | 0.98 | 0.98 | 0.92 |
logarithmic loss | 0.01 | 0.01 | 0.02 |
Matthews coef | 0.95 | 0.94 | 0.73 |
Notes. The upper bound of the uncertainty of these metrics, calculated as the standard deviation from the five fold cross-validation process during the training, is 0.03. The superscripts a and b indicate that the model was evaluated on GUMS selected samples with G < 12.5 mag, and G <19 mag respectively.
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