Kavli Affiliate: Subo Dong | Summary:Kilonovae (KNe) are the electromagnetic signatures of neutron star mergers and are likely the dominant site of cosmic $r$-process nucleosynthesis. However, their intrinsic rate remains poorly constrained due to a paucity of confirmed events. We use the All-Sky Automated Survey for Supernovae (ASAS-SN) to place limits on the rate of […]
Continue.. ASAS-SN Rates IV: Constraints on the Kilonova Rate