The possible electromagnetic counterparts of the first high-probability NSBH merger LIGO/Virgo S190814bv
Hao Wei,Minzi Feng
Table 1. The Fermi GBM short GRBs probably associated with the real NSBH merger ‘S’ corresponding to LIGO/Virgo S190814bv. We classify them as ‘Gold’ candidates or ‘Silver’ candidates. Note that some of these GRBs have not been reported in GCN, but can be found in the published Fermi GBM GRB Catalog [52, 53]. These results are for case (I). See the text for details.
GRB nameGRB nameRADECError radius T90ΔtθΔθ (NE2001)Δθ (YMW16)Candidate
(GRByymmddfff) (GRByymmddx)  (J2000, hms)  (J2000, dms) (deg)(s)(year)(deg)(deg)(deg)(G/S)
GRB100107074GRB100107A00:25:14.4−21:14:245.970.576 ± 0.4659.6014.8132.9650.865Gold
GRB14112208700:38:50.4−20:01:1210.901.280 ± 0.9454.7285.0080.4481.024Gold
GRB101214748GRB101214A00:02:45.6−28:16:125.562.240 ± 2.0848.6668.5491.1603.155Gold
GRB090108322GRB090108B00:01:36.0−32:54:008.300.192 ± 0.14310.59711.2153.0435.250Gold

GRB081213173GRB08121300:51:36.0−33:54:0013.200.256 ± 0.28610.6699.3421.1433.356Silver
GRB120524134GRB120524A23:52:36.0−15:36:3610.450.704 ± 0.4667.22414.2267.4819.301Silver
GRB120314412GRB120314A01:11:33.6−48:43:4817.821.280 ± 1.0867.41824.59217.75619.601Silver
GRB12092675301:38:26.4−45:34:4821.323.072 ± 2.0646.88123.86017.27819.054Silver
GRB14010987701:36:21.6−25:03:0037.453.328 ± 2.5605.59313.1747.2398.841Silver