Table 4.
AMPEL sample channel parameter settings and rerun statistics for cases when only transients close to host galaxies of z < 0.1 are included.
| 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) | ||||||
| 85 | 0.3 | 4 | Persistent | Good | Nominal | 21 | 261 | 0.750 | 0.000 | 19 | 143 | 0.714 | 0.000 |
| 34 | 0.5 | 2 | Multinight | Excellent | Nominal | 20 | 231 | 0.867 | 0.067 | 18 | 136 | 0.846 | 0.077 |
| 16 | 0.5 | 2 | New | All | Nominal | 17 | 160 | 0.923 | 0.385 | 15 | 101 | 0.909 | 0.273 |
| 29 | 0.5 | 4 | New | Excellent | Nominal | 4 | 9 | 1.000 | 0.000 | 3 | 6 | 1.000 | 0.000 |
| 84 | 0.3 | 8 | Multinight | All | Moderate | 11 | 32 | 0.333 | 0.000 | 10 | 24 | 0.375 | 0.000 |
| 28 | 0.5 | 2 | New | Excellent | Nominal | 15 | 117 | 0.917 | 0.333 | 14 | 79 | 0.909 | 0.273 |
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 the same 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 to −10 days with respect to the peak.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.