Review Article

The Observer’s Guide to the Gamma-Ray Burst Supernova Connection

Table 2

GRB-SN master Table 1: -ray properties.

( erg)(keV)(erg )
GRB SNType (s)      

970228GRB0.695561.6 (0.12)195 (64)
980326GRB0.48 (0.09)935 (36)
9804251998bwGRB0.00867180.000086 (0.000002)55 (21)
990712GRB0.4331190.67 (0.13)93 (15)
991208GRB0.70636022.3 (1.8)313 (31)
000911GRB1.058550067 (14)1859 (371)
0111212001keGRB0.362477.8 (2.1)793 (265)
020305
020405GRB0.689864010 (0.9)612 (10)
020410>1600
020903GRB0.25063.30.0011 (0.0006)3.37 (1.79)
0212112002ltGRB1.0042.81.12 (0.13)127 (52)
0303292003dhGRB0.1686722.761.5 (0.3)100 (23)
030723<0.023
030725
0312032003lwGRB0.10536370.0086 (0.004)<200
040924GRB0.8582.390.95 (0.09)102 (35)
041006GRB0.716183 (0.9)98 (20)
050416AINT0.65282.40.1 (0.01)25.1 (4.2)
050525A2005ncGRB0.6068.842.5 (0.43)127 (10)
050824GRB0.828125
0602182006ajGRB0.0334221000.0053 (0.0003)4.9 (0.3)
060729GRB0.54281151.6 (0.6)>50
060904BGRB0.70291922.4 (0.2)163 (31)
070419AINT0.9705116≈0.16
080319BGRB0.9371124.86114 (9)1261 (65)
0810072008hwGRB0.52959.010.15 (0.04)61 (15)
090618GRB0.54113.3425.7 (5)211 (22)
0911272009nzGRB0.490447.421.5 (0.2)35.5 (1.5)
100316D2010bhGRB0.05921300>0.005926 (16)
100418AGRB0.623980.0990 (0.0630)29 (2)
101219B2010maGRB0.55185510.42 (0.05)70 (8)
101225AULGRB0.84770001.2 (0.3)38 (20)
111209A2011klULGRB0.677021000058.2 (7.3)520 (89)
111211A0.478
111228AGRB0.71627101.24.2 (0.6)58.4 (6.9)
120422A2012bzGRB0.282535.40.024 (0.008)<72
120714B2012ebINT0.39841590.0594 (0.0195)101.4 (155.7)
120729AGRB0.871.52.3 (1.5)310.6 (31.6)
130215A2013ezGRB0.59765.73.1 (1.6)155 (63)
130427A2013cqGRB0.339916381 (10)1028 (50)
130702A2013dxINT0.14558.8810.064 (0.013)15 (5)
130831A2013fuGRB0.47932.50.46 (0.02)67 (4)
140606BGRB0.38422.780.347 (0.02)801 (182)
150518A0.256
150818AINT0.282123.30.1 (0.02)128 (13)

.
-ray properties calculated by [85] for a redshift range of .
GRB: GRB-SN associated with a low-luminosity GRB ( erg ); INT: GRB-SN associated with an intermediate-luminosity GRB ( erg ); GRB: GRB-SN associated with a high-luminosity GRB ( erg ); ULGRB: GRB-SN associated with an ultra-long-duration GRB (see Section 3).