Table 3.
AMPEL sample channel parameter settings and rerun statistics.
Channel | RealBogus | Detections | History | Image | Gaia | SNe Ia | Detections | Phase(< 0) | Phase(< − 10) | SNe Ia | Detections | Phase(< 0) | Phase(< − 10) |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
(all) | (all) | (all) | (all) | (no AGN) | (no AGN) | (no AGN) | (no AGN) | ||||||
11 | 0.5 | 4 | Multinight | Good | Nominal | 125 | 1857 | 0.956 | 0.067 | 120 | 1514 | 0.953 | 0.047 |
26 | 0.3 | 4 | New | Excellent | Nominal | 36 | 293 | 1.000 | 0.296 | 35 | 257 | 1.000 | 0.308 |
34 | 0.5 | 2 | Multinight | Excellent | Nominal | 128 | 2479 | 0.944 | 0.079 | 123 | 1964 | 0.941 | 0.059 |
18 | 0.5 | 6 | New | All | Nominal | 2 | 34 | 0.000 | 0.000 | 2 | 28 | 0.000 | 0.000 |
77 | 0.3 | 4 | Persistent | All | Moderate | 131 | 10 672 | 0.832 | 0.000 | 126 | 9705 | 0.824 | 0.000 |
51 | 0.3 | 4 | New | Good | Nominal | 39 | 357 | 1.000 | 0.321 | 37 | 311 | 1.000 | 0.308 |
57 | 0.3 | 4 | Persistent | Good | Nominal | 130 | 3078 | 0.830 | 0.000 | 125 | 2351 | 0.822 | 0.000 |
64 | 0.3 | 8 | Multinight | Good | Nominal | 76 | 580 | 0.554 | 0.000 | 74 | 524 | 0.556 | 0.000 |
1 | 0.3 | 2 | New | Good | Nominal | 110 | 2968 | 0.987 | 0.557 | 106 | 2562 | 0.987 | 0.533 |
28 | 0.5 | 2 | New | Excellent | Nominal | 95 | 1833 | 0.985 | 0.485 | 92 | 1547 | 0.985 | 0.462 |
4 | 0.5 | 2 | New | Good | Nominal | 103 | 2286 | 0.986 | 0.514 | 99 | 1909 | 0.985 | 0.485 |
10 | 0.5 | 2 | Multinight | Good | Nominal | ||||||||
59 | 0.3 | 4 | Persistent | Good | Moderate | ||||||||
10+59 | 134 | 11 112 | 0.926 | 0.084 | 129 | 9973 | 0.923 | 0.055 |
Notes. Columns 2–6 show settings used for parameters in Table 2, Cols. 7–10 show statistics including all targets, and Cols. 11–14 show statistics when excluding AGN-associated candidates. The phase estimates describe the fraction of the matched SNe Ia with a good peak phase estimate that were accepted by the channel either prior to light curve peak or prior to −10 days with respect to peak light.
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