Table 6.
IceCube HESE and EHE events and Pan-STARRS1 observations from 2016−2017.
| Neutrino event | Epoch | Energy alert | αJ2000 | δJ2000 | 90% error | Pan-STARRS1 observations | mdepth, iP1 | Number of | |
|---|---|---|---|---|---|---|---|---|---|
| (MJD) | type | (°) | (°) | (°) | Start | End | (mag) | transients | |
| IceCube-160427A | 57 505.24481 | HESE | 240.3 | 9.7 | 0.45 − 0.54 | 57 508.50 | 57 550.46 | 22.5 | 19 |
| IceCube-160731A | 57 600.07990 | HESE+EHE | 214.5 | −0.3 | 0.75 | 57 600.32 | 57 626.28 | 22 | 11 |
| IceCube-160806A | 57 606.51496 | EHE | 122.8 | −0.8 | 0.5 | Not visible | − | − | − |
| IceCube-160814A | 57 614.90688 | HESE | 200.3 | −32.4 | 1.2 − 3.0 | Not visible | − | − | − |
| IceCube-161103A | 57 695.38022 | HESE | 40.8 | 12.6 | 0.65 − 1.1 | 57 695.47 | 57 702.36 | 22 | 7 |
| IceCube-161210A | 57 732.83797 | EHE | 46.6 | 15.0 | 0.4 − 1.1 | Not observed | − | − | − |
| IceCube-170312A | 57 824.57615 | HESE | 305.2 | −26.6 | 0.5 | Not observed | − | − | − |
| IceCube-170321A | 57 833.31413 | EHE | 98.3 | −15.0 | 1.2 | 57 834.27 | 57 859.27 | 22 | 2 |
| IceCube-170506A | 57 879.52565 | HESE | 221.8 | −26.0 | 2.0 − 3.0 | Not observed | − | − | − |
| IceCube-170922A | 58 018.87118 | EHE | 77.4 | 5.7 | 0.3 − 0.95 | Not observed | − | − | − |
| IceCube-171015A | 58 041.06562 | HESE | 162.9 | −15.4 | 1.6 − 2.6 | Not visible | − | − | − |
| IceCube-171028A | 58 054.35295 | HESE | 67.5 | −69.8 | > 7 − 28 | Not observed | − | − | − |
| IceCube-171106A | 58 063.77754 | EHE | 340.0 | 7.4 | 0.25 − 0.7 | 58 065.34 | 58 075.34 | 22.5 | 2 |
Notes. The events labelled “Not visible” have IceCube positions in the daytime sky. Events marked “Not observed” were either due to weather, Moon encroachment or other reasons not to observe the field. The information on the final reconstructed sky locations of the IceCube neutrinos are taken from the IceCube catalogue of alert events up through IceCube-170922A (https://icecube.wisc.edu/science/data/TXS0506_alerts), or from the IceCube Collaboration (2017a,b,c). The number of transients are those within the 90% error localisation.
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