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.
Modeling, Systems Engineering, and Project Management for Astronomy VI , year = 2014, editor =
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A convLSTM classifier identifies lensed SNe Ia in simulated LSST-like time series, reaching ~60% true-positive rate at O(10^{-4}) false-positive rate by the seventh epoch even after adding realistic PSF variations and foreground SN contaminants.
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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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HOLISMOKES XXI: Detecting strongly lensed type Ia supernovae from time series of multi-band LSST-like imaging data -- Part II
A convLSTM classifier identifies lensed SNe Ia in simulated LSST-like time series, reaching ~60% true-positive rate at O(10^{-4}) false-positive rate by the seventh epoch even after adding realistic PSF variations and foreground SN contaminants.