Table A.1.
List of GRBs observed by MAGIC (under acceptable conditions) between 2013 and 2019.
| GRB | Redshift | Instrument | T90 | T0 | Tstart | Tdelay | Zenith angle |
|---|---|---|---|---|---|---|---|
| name | (position) | [s] | [UTC] | [UTC] | [s] | [deg] | |
| 130502A | Swift-BAT | 3 | 17:50:30 | 20:57:03 | 11193 | 33.9-40.1 | |
| 130504A | Swift-BAT | 50 | 02:05:34 | 02:13:09 | 455 | 44.7-56.5 | |
| 130606A | 5.913 | Swift-BAT | 277 | 21:04:39 | 21:15:28 | 649 | 1.7-46.1 |
| 130612A | 2.006 | Swift-BAT | 5.6 | 03:22:22 | 03:23:08 | 46 | 38.0-53.0 |
| 130701A | 1.155 | Swift-BAT | 4.4 | 04:17:43 | 04:18:32 | 49 | 15.9-22.6 |
| 130903A | INTEGRAL | 69 | 00:47:20 | 03:57:32 | 11412 | 51.9-62.8 | |
| 131030A | 1.295 | Swift-BAT | 41 | 20:56:19 | 20:56:45 | 26 | 33.7-39.7 |
| 140430A | 1.60 | Swift-BAT | 174 | 20:33:36 | 20:52:06 | 1110 | 45.6-73.3 |
| 140709A | Swift-BAT | 98.6 | 01:13:41 | 03:22:13 | 7712 | 24.6-37.0 | |
| 140930B | Swift-BAT | 0.84 | 19:41:42 | 21:10:05 | 5303 | 18.8-51.4 | |
| 141026A | 3.35 | Swift-BAT | 146 | 02:36:51 | 02:38:27 | 96 | 16.3-54.1 |
| 141220A | 1.32 | Swift-BAT | 7.21 | 06:02:52 | 06:03:47 | 55 | 18.9-24.0 |
| 150213A | Fermi-GBM | 4.1 | 00:01:48 | 00:03:08 | 80 | 48.2-60.6 | |
| 150428A | Swift-BAT | 53.2 | 01:30:40 | 01:32:11 | 91 | 27.0-57.7 | |
| 150428B | Swift-BAT | 131 | 03:12:03 | 03:13:03 | 60 | 27.0-57.7 | |
| 150819A | Swift-BAT | 52.1 | 00:50:08 | 02:11:51 | 4903 | 37.4-54.4 | |
| 151118A | Swift-BAT | 23.4 | 03:06:30 | 03:07:14 | 44 | 42.8-57.4 | |
| 151215A | 2.59 | Swift-BAT | 17.8 | 03:01:28 | 03:01:58 | 30 | 15.8-58.0 |
| 160119A | Swift-BAT | 116 | 03:06:07 | 03:17:09 | 662 | 13.2-58.7 | |
| 160310A | Fermi-LAT | 18.2 | 00:22:57 | 20:30:16 | 72439 | 35.5-40.9 | |
| 160313A | Swift-BAT | 42.6 | 02:37:14 | 02:39:01 | 107 | 30.3-53.3 | |
| 160504A | Swift-BAT | 53.9 | 19:30:36 | 20:56:29 | 5153 | 26.9-33.7 | |
| 160509A | 1.17 | Fermi-LAT | 370 | 08:59:04 | 21:21:07 (+2d) | 217323 | 49.2-72.2 |
| 160623A | 0.367 | Fermi-LAT | 50 | 05:00:34 | 02:05:31 | 75897 | 27.0-54.7 |
| 160625B | 1.406 | Fermi-LAT | 460 | 22:43:24 | 23:29:38 | 2774 | 21.8-54.9 |
| 160821B | 0.16 | Swift-BAT | 0.48 | 22:29:13 | 22:29:37 | 24 | 33.4-43.6 |
| 160910A | Fermi-GBM | 24.3 | 17:19:38 | 20:21:54 | 10936 | 45.4-72.9 | |
| 160927A | Swift-BAT | 0.48 | 18:04:49 | 20:03:00 | 7091 | 32.0-58.8 | |
| 161229A | Fermi-GBM | 33.5 | 21:03:48 | 23:05:54 | 7326 | 22.0-26.1 | |
| 170728B | Swift-BAT | 47.7 | 23:03:19 | 23:03:58 | 39 | 41.8-52.7 | |
| 170921B | Fermi-GBM | 39.4 | 04:02:11 | 04:48:04 | 2753 | 48.4-60.6 | |
| 171020A | 1.87 | Swift-BAT | 41.9 | 23:07:09 | 23:08:37 | 88 | 13.5-34.9 |
| 171210A | Fermi-LAT | 12 | 11:49:15 | 20:33:11 | 31436 | 30.9-61.9 | |
| 180512A | Swift-BAT | 24.0 | 22:01:46 | 22:03:11 | 85 | 7.6-38.4 | |
| 180715A | Swift-BAT | 0.68 | 18:07:05 | 21:27:24 | 12019 | 27.9-34.5 | |
| 180720C | Swift-BAT | 124.2 | 22:23:57 | 22:25:44 | 107 | 55.3-55.4 | |
| 180904A | Swift-BAT | 5.39 | 21:28:32 | 21:30:07 | 95 | 23.7-60.2 | |
| 181225A | Fermi-LAT | 41.5 | 11:44:10 | 19:56:06 (+1d) | 115916 | 46.7-62.6 | |
| 190106B | Fermi-GBM | 11.8 | 20:47:10 | 20:49:13 | 123 | 60.0-60.4 | |
| 190114C | 0.425 | Swift-BAT | 25* | 20:57:03 | 20:58:01 | 58 | 55.6-80.0 |
| 190829A | 0.078 | Swift-BAT | 62.9 | 19:55:53 | 02:23:48 (+2d) | 109624 | 37.7-59.6 |
| 191004A | Swift-BAT | 2.44 | 18:07:02 | 00:42:30 | 23728 | 65.4-69.9 |
Notes. The GRB redshift, when measured, is reported in the second column. The third column reports the name of the satellite which provided the sky coordinates (e.g. through GCN Notices or Circulars). The forth column reports the prompt emission duration T90. The fifth and sixth columns give the time of the trigger T0 and the time Tstart when MAGIC started the observations. The delay Tdelay(in seconds) is computed as the difference between the start time and the trigger time. The last column reports the zenith angle range related to each GRB observation. *Nominally, the T90 of GRB 190114C measured by and GBM is > 300 s. However, most of the emission recorded by and GBM was interpreted as afterglow radiation. The end of the prompt emission can be roughly identified with the end of flux variability, which occurs approximately at 25 s.
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