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.
and Butler, Nathaniel R
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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.