Given TeV emission similar to GRB 090510, CTA could detect short-GRB counterparts of gravitational-wave mergers even when follow-up starts more than an hour after the event.
Quantum Grav] 10.1088/0264-9381/25/11/114051 , http://adsabs.harvard.edu/abs/2008CQGra..25k4051A 25, 114051
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Gravitational-wave follow-up with CTA after the detection of GRBs in the TeV energy domain
Given TeV emission similar to GRB 090510, CTA could detect short-GRB counterparts of gravitational-wave mergers even when follow-up starts more than an hour after the event.