Table 2
Magnitude dependence of object-detection probabilities for the functional-baseline rejection parameters.
| G range | P G ∗ | P G ∗ ∗ → ∗ | P G ∗ ∗ → ∗ ∗ | P G,CR | P G,SP |
| [mag] | [%] | [%] | [%] | [%] | [%] |
|
|
|||||
| 12.5–13.5 | 100.000 | 99.917 | 99.188 | 8.584 | 15.781 |
| 13.5–14.5 | 100.000 | 99.929 | 99.302 | 11.218 | 12.091 |
| 14.5–15.5 | 100.000 | 99.936 | 99.263 | 4.589 | 6.346 |
| 15.5–16.5 | 100.000 | 99.946 | 98.763 | 11.957 | 1.048 |
| 16.5–17.5 | 100.000 | 99.886 | 99.027 | 2.780 | 0.454 |
| 17.5–18.5 | 100.000 | 99.808 | 99.121 | 7.646 | 2.651 |
| 18.5–19.5 | 99.999 | 99.326 | 98.660 | 3.871 | – |
| 19.5–20.0 | 99.831 | 94.306 | 96.200 | – | – |
|
|
|||||
| 12.5–20.0 | 99.961 | 98.417 | 98.271 | 6.349 | 3.401 |
Notes. The symbol “–” indicates the absence of faint cosmic rays and solar protons in our prompt-particle-event catalogues, as explained in Sect. 3.4. The magnitude-averaged star-detection probabilities PG ∗, PG ∗ ∗ → ∗, and PG ∗ ∗ → ∗ ∗ in the last line are weighted with the Galaxy-model weights wG from Table 1. The functional-baseline detection performance is not compatible with the minimum detection percentages defined in Table 1.
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