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 Covino, Stefano and Nappo, Francesco and Vergani, Susanna D
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Empirical zero-point constants for Gaia bolometric corrections are derived as weighted averages 0.8677, 1.0449, and 2.0510 mag for G, GBP, and GRP from 88 stars, yielding corresponding magnitude zero-points via IAU definitions.
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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Spectroscopic Bolometric Corrections and Empirical Zero-point Constants of \textit{Gaia} Magnitudes, $G$, $G_{\rm BP}$, and $G_{\rm RP}$, from \textit{Gaia} XP Spectra
Empirical zero-point constants for Gaia bolometric corrections are derived as weighted averages 0.8677, 1.0449, and 2.0510 mag for G, GBP, and GRP from 88 stars, yielding corresponding magnitude zero-points via IAU definitions.