941 days after the neutron star merger, for a total exposure time of~ 96 ks. The observations
were taken in 4 distinct exposures of~ 24ks,~ 16ks,~ 19ks, and~ 36 ks, respectively (ObsID
21323, 23183, 23184 and 23185; PI Margutti; program 20500299, for which we waived
proprietary data rights). The observations were taken on March 09, 2020 through March 15,
2020. We reported the results from our first observation (ObsID 21323) in Hajela et al.(GCN …