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Table 2.

GRB detection rates.

LONG SHORT
Total S X X-only Total S X X-only

HP 195 21 + 22 $ 195^{+22}_{-21} $ 147 11 + 13 $ 147^{+13}_{-11} $ 131 19 + 17 $ 131^{+17}_{-19} $ 51 13 + 12 $ 51^{+12}_{-13} $ 19 3 + 5 $ 19^{+5}_{-3} $ 19 3 + 5 $ 19^{+5}_{-3} $ 0 . 3 0.2 + 0.4 $ 0.3^{+0.4}_{-0.2} $ < 0.1
Const. A 1565 244 + 292 $ 1565^{+292}_{-244} $ 772 61 + 67 $ 772^{+67}_{-61} $ 1517 251 + 289 $ 1517^{+289}_{-251} $ 796 204 + 221 $ 796^{+221}_{-204} $ 191 28 + 40 $ 191^{+40}_{-28} $ 188 28 + 38 $ 188^{+38}_{-28} $ 7 4 + 5 $ 7^{+5}_{-4} $ < 3
Const. B 2468 452 + 531 $ 2468^{+531}_{-452} $ 996 64 + 119 $ 996^{+119}_{-64} $ 2455 460 + 529 $ 2455^{+529}_{-460} $ 1473 375 + 419 $ 1473^{+419}_{-375} $ 327 61 + 78 $ 327^{+78}_{-61} $ 322 58 + 76 $ 322^{+76}_{-58} $ 18 10 + 8 $ 18^{+8}_{-10} $ < 7

Notes. Number of events per year expected with HERMES (HP and Constellation) for the short and long classes. For each GRB class, the table reports the total rate and the partial rates on the single instruments (S – all events detected by S; X – all events detected by X; X-only – all events detected only by the X instrument). The difference in configurations A and B for the Constellation is the FoV of the single satellite (see Table 1).

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