Table A.2.
H.E.S.S. Follow-up observations triggered by Fermi/GBM.
| Name | T0 | delay (min) | Analysis configuration |
|---|---|---|---|
| GRB 150127589 | 2015-01-27 14:08:26 | 588.5 | stereo loose |
| GRB 150422703 | 2015-04-22 16:52:33 | 188.7 | hybrid loose |
| GRB 160113398 | 2016-01-13 09:32:30 | 997.2 | stereo loose |
| GRB 160822672 | 2016-08-22 16:07:40 | 144.1 | hybrid loose |
| GRB 160825799 | 2016-08-25 19:10:49 | 94.5 | mono loose |
| GRB 160825799 | 205.4 | mono loose | |
| GRB 170402961 | 2017-04-02 23:03:25 | 262.5 | stereo loose |
| GRB 170730133 | 2017-07-30 03:11:44 | 1206.9 | hybrid loose |
| GRB 170826819 | 2017-08-26 19:38:56 | 92.4 | hybrid loose |
| GRB 171112868 | 2017-11-12 20:50:17 | 22.4 | hybrid loose |
| GRB 180522607 | 2018-05-22 14:34:38 | 737.4 | hybrid loose |
| GRB 180906759 | 2018-09-06 18:12:25 | 1.1 | hybrid loose |
| GRB 190306943 | 2019-03-06 22:37:43 | 84.5 | stereo loose |
| GRB 190306943 | 237.3 | stereo loose | |
| GRB 190507970 | 2019-05-07 23:16:29 | 29.0 | hybrid loose |
| GRB 190727668 | 2019-07-27 16:01:52 | 107.4 | hybrid loose |
Notes. The Fermi/GBM name identifier is used here for uniformity as many of these GRBs do not have an official GCN name. The second column corresponds to the time of the onset of the burst (T0), the third column indicates the delay of the H.E.S.S. observation in minutes and the fourth column indicates the analysis configuration (see Sect. 4). Columns without T0 values correspond to subsequent H.E.S.S. observations of the GRB in the previous column with provided T0. In Sect. 4, the results of UL maps for these GRBs are detailed.
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