Table 2.
Results of synthetic insertion tests.
| FRB | 180924 | 181112 | 190102 | Combined | ||||
|---|---|---|---|---|---|---|---|---|
| Band | g | I | g | I | g | I | g | I |
| Limit at burst position (mag) | 25.1 | 23.6 | 25.2 | 24.6 | 26.4 | 25.2 | – | – |
| Probability of non-detection | ||||||||
| Type Ia | 34% | 12% | 44% | 34% | 78% | 88% | 12% | 4% |
| Type Ib | 94% | 54% | 91% | 91% | 99% | 99% | 85% | 49% |
| Type Ic | 94% | 49% | 88% | 80% | 98% | 98% | 82% | 39% |
| Type IIn | 40% | 41% | 34% | 47% | 39% | 65% | 6% | 13% |
| Type II-L | 69% | 48% | 78% | 79% | 63% | 76% | 34% | 29% |
| Type II-P | 89% | 73% | 75% | 89% | 74% | 90% | 50% | 59% |
Notes. The probability of non-detection is the estimated probability that, if a supernova of this type did occur in the given host galaxy coincident with the FRB emission, it would not be found. The combined column gives the estimated probability that, if a given SN type occurred in all three difference images, it would go undetected.
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