Advances in Astronomy

Review Article

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

Table 3

GRB-SN master Table 2: SN properties.
      (mag)(mag)(d)(erg )(d)(mag)( erg)()()(km )   
GRB SNTypeS?GradeFilters
970228 GRB0.695 C             
980326 GRB  D             
9804251998bwGRB0.00866SA15.160.8020–306–100.3–0.618000 
990712 GRB0.4331 C       
991208 GRB0.7063 E       
000911 GRB1.0585 E             
0111212001keGRB0.362SB   ~~17  
020305    E             
020405 GRB0.68986 C       
020410    D             
020903 GRB0.2506SB       
0212112002ltGRB1.004SB       
0303292003dhGRB0.16867SA12.750.7020–505–100.4–0.620000
030723    D             
030725    E             
0312032003lwGRB0.10536SA17.330.6218000
040924 GRB0.858 C             
041006 GRB0.716 C       
050416A INT0.6528 D             
050525A2005ncGRB0.606SB    
050824 GRB0.8281 E       
0602182006ajGRB0.03342SA10.420.8320000
060729 GRB0.5428 D       
060904B GRB0.7029 C       
070419A GRB0.9705 D             
080319B GRB0.9371 C       
0810072008hwGRB0.5295SB   ~~12 12600
090618 GRB0.54 C    
0911272009nzGRB0.49044SB   ~1.2 ×  ~15~0.517000
100316D2010bhGRB0.0592SA8.760.8935000
100418A INT0.6239 D/E             
101219B2010maGRB0.55185SA/B   11.800.99 
101225A ULGRB0.847 D       
111209A2011klULGRB0.67702 A/B   14.800.7820–903–5 21000
111211A  0.478SB/C             
111228A  0.71627 E             
120422A2012bzGRB0.28253SA14.450.6220500
120714B2012eb 0.3984SB             
120729A GRB0.8 D/E         
130215A2013ezGRB0.597SB        0.25–0.3060000.6–0.75
130427A2013cqGRB0.3399SB      35000
130702A2013dxINT0.145SA12.940.8521300
130831A2013fuGRB0.479SA/B       
140606B GRB0.384SA/B      19800
150518A  0.256 C/D             
150818A INT0.282SB             
—2009bbRel IcBL0.009987S—   15000
—2012apRel IcBL0.012141S    13000
S denotes one or more spectra of the SN were obtained.
Grades are from Hjorth and Bloom (2012): A: strong spectroscopic evidence. B: a clear light curve bump as well as some spectroscopic evidence resembling a GRB-SN. C: a clear bump consistent with other GRB-SNe at the spectroscopic redshift of the GRB. D: a bump, but the inferred SN properties are not fully consistent with other GRB-SNe or the bump was not well sampled or there is no spectroscopic redshift of the GRB. E: a bump, either of low significance or inconsistent with other GRB-SNe.
denotes exact, -corrected rest-frame filter observable.
fixed during fit.
and denote the filter-averaged luminosity () and stretch () factors relative to SN 1998bw.