Table 2.

Accuracy of the threshold-based anomaly detector for different thresholds, and of k-means anomaly detector method. Each method (columns) is evaluated for test sets (rows) of pre-merger galaxies divided according to their flux ratio between the central galaxy and the brightest neighbour (Fc/Fn). Thresholds 1, 2, and 3 represent the three thresholds defined as the value that contains, respectively, 85, 90, and 95 per cent of the training galaxies within the generative distribution. The last column indicates the accuracy according to the k-means clustering method.

Accuracy of the anomaly detector
Threshold
123k-means
Fr < 1.596  per cent93  per cent86  per cent91  per cent
1.5 < Fr < 294  per cent90  per cent76  per cent93  per cent
Fr > 275  per cent66  per cent48  per cent39  per cent
Accuracy of the anomaly detector
Threshold
123k-means
Fr < 1.596  per cent93  per cent86  per cent91  per cent
1.5 < Fr < 294  per cent90  per cent76  per cent93  per cent
Fr > 275  per cent66  per cent48  per cent39  per cent
Table 2.

Accuracy of the threshold-based anomaly detector for different thresholds, and of k-means anomaly detector method. Each method (columns) is evaluated for test sets (rows) of pre-merger galaxies divided according to their flux ratio between the central galaxy and the brightest neighbour (Fc/Fn). Thresholds 1, 2, and 3 represent the three thresholds defined as the value that contains, respectively, 85, 90, and 95 per cent of the training galaxies within the generative distribution. The last column indicates the accuracy according to the k-means clustering method.

Accuracy of the anomaly detector
Threshold
123k-means
Fr < 1.596  per cent93  per cent86  per cent91  per cent
1.5 < Fr < 294  per cent90  per cent76  per cent93  per cent
Fr > 275  per cent66  per cent48  per cent39  per cent
Accuracy of the anomaly detector
Threshold
123k-means
Fr < 1.596  per cent93  per cent86  per cent91  per cent
1.5 < Fr < 294  per cent90  per cent76  per cent93  per cent
Fr > 275  per cent66  per cent48  per cent39  per cent
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