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Table 3

Simulation results.

z f gain,w f loss,w f gain f loss dz N app

Thermonuclear Supernovae
z ≤ 0.25 0.019 0.025 0.039 0.046 0.091 540
0.25 < z ≤ 0.50 0.098 0.023 0.096 0.043 0.12 2894
0.50 < z ≤ 0.75 0.096 0.032 0.10 0.052 0.084 3102
0.75 < z ≤ 1.00 0.057 0.017 0.078 0.022 0.074 1759
1.00 < z ≤ 1.25 0.038 0.0045 0.061 0.0056 0.095 358
1.25 < z ≤ 1.50 0.26 0.0 0.50 0.00 0.082 20

z ≤ 1.5 0.082 0.024 0.042 0.071 0.098 8673

Core-collapse Supernovae
z ≤ 0.25 0.0079 0.0060 0.015 0.013 0.078 1676
0.25 < z ≤ 0.50 0.020 0.085 0.038 0.084 0.12 3319
0.50 < z ≤ 0.75 0.041 0.12 0.067 0.13 0.083 2428
0.75 < z ≤ 1.00 0.026 0.085 0.032 0.12 0.094 1172
1.00 < z ≤ 1.25 0.0034 0.029 0.0042 0.047 0.12 472
1.25 < z ≤ 1.50 0.0 0.014 0.00 0.027 0.16 367

z ≤ 1.5 0.022 0.075 0.084 0.037 0.11 9434

Notes. fgain,w/floss,w are the misclassification ratios weighted by subtype frequency and fgain/floss are the unweighted misclassification ratios. dz is the redshift variance (based on the fitted redshift from the typing code compared to the true redshift of the supernova) for the specific bin and Napp is the apparent number of simulated supernovae of the given type in the bin.

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