Table 2
Cumulative number of each SN type associated within the error radius of Fermi-GRBs at different time intervals after the trigger time.
| Δt (days) | 10 | 20 | 30 | 40 | 50 | 60 | 70 | 80 | 90 | 100 | 110 | 120 | 150 | 200 | 300 | 400 | 500 | rx (%) |
|
|
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| NIb / c(Δt) | 8 | 9 | 9 | 13 | 13 | 15 | 17 | 18 | 18 | 20 | 21 | 26 | 30 | 42 | 68 | 81 | 96 | 12 |
| NIa(Δt) | 10 | 23 | 30 | 42 | 51 | 64 | 77 | 85 | 98 | 108 | 118 | 131 | 164 | 213 | 338 | 440 | 519 | 66 |
| NIIp(Δt) | 2 | 4 | 8 | 14 | 16 | 19 | 19 | 21 | 22 | 26 | 27 | 30 | 39 | 54 | 82 | 103 | 124 | 16 |
| NIIn(Δt) | 1 | 2 | 4 | 6 | 8 | 9 | 9 | 9 | 10 | 11 | 11 | 11 | 14 | 21 | 30 | 38 | 51 | 6 |
|
|
||||||||||||||||||
| Ntot(Δt) | 31 | 67 | 98 | 136 | 166 | 209 | 240 | 260 | 288 | 314 | 338 | 378 | 471 | 627 | 893 | 1139 | 1399 | 100 |
Notes. In the first row the considered time intervals (in days) are listed. In the following rows the number of possible associations for each type of SN, respectively, Ib/c, Ia, IIp, and IIn, and the total number of SNe, for each considered time interval, are listed. In the last column the percentage rx of the total number of each SN type over the total sample is shown.
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