Simulations predict LSST will detect roughly 5 on-axis and 11 orphan afterglows per year, Roman is suited for faint events, but fewer than 1.4 events per year are expected in the aLIGO O5 range across jet models.
10.1051/0004-6361/201526112
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Overview of SKAO's role in radio follow-up of GW events, GRB afterglows, and kilonovae for system characterization and population studies.
citing papers explorer
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Short-Duration Gamma-ray Burst and Afterglow Rates in the Rubin and Roman Era
Simulations predict LSST will detect roughly 5 on-axis and 11 orphan afterglows per year, Roman is suited for faint events, but fewer than 1.4 events per year are expected in the aLIGO O5 range across jet models.
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Gamma-ray Bursts and Kilonovae from Gravitational Wave Events
Overview of SKAO's role in radio follow-up of GW events, GRB afterglows, and kilonovae for system characterization and population studies.