Using a re-fitted BNS-sGRB population model and AfterglowPy simulations, the paper forecasts ~5 on-axis and ~11 orphan afterglows per year for LSST, and <1.4 joint optical-GW afterglows per year in LIGO O5.
Weizmann and Farah, Amanda M
2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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2026 2representative citing papers
Hybrid SPA-plus-FFT frequency-domain version of SEOBNRv5THM for quasi-circular spin-aligned BNS systems matches time-domain baseline accuracy while cutting computational cost for long signals.
citing papers explorer
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Short-Duration Gamma-ray Burst and Afterglow Rates in the Rubin and Roman Era
Using a re-fitted BNS-sGRB population model and AfterglowPy simulations, the paper forecasts ~5 on-axis and ~11 orphan afterglows per year for LSST, and <1.4 joint optical-GW afterglows per year in LIGO O5.
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Speed and accuracy for long signals: Frequency-domain effective-one-body waveforms for compact binary coalescences
Hybrid SPA-plus-FFT frequency-domain version of SEOBNRv5THM for quasi-circular spin-aligned BNS systems matches time-domain baseline accuracy while cutting computational cost for long signals.