H.E.S.S. developed scheduling and alert tools for gravitational wave follow-up and used them to observe GW170814, GW170817, and S190512at, finding no significant very-high-energy gamma-ray emission.
Astroparticle Physics 32.5 (2009): 231-252
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Searches for counterparts of gravitational waves at very high energies with H.E.S.S
H.E.S.S. developed scheduling and alert tools for gravitational wave follow-up and used them to observe GW170814, GW170817, and S190512at, finding no significant very-high-energy gamma-ray emission.