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Table 2

Supernova components for GRBs with redshift  <1.0.

Short bursts Intermediate bursts Long bursts

GRB SN? Reference GRB SN? Reference GRB SN? Reference

050509B N Hjorth et al. 2005a 050223 050826
050813 N Ferrero et al. 2007 050416A Y Soderberg et al. 2007 060202
051221A N Soderberg et al. 2006 050525A Y Della Valle et al. 2006b 060218 Y Pian et al. 2006
060502B N Kann et al. 2008 050724 N Berger et al. 2005c 060602A
061006 050824 Y Sollerman et al. 2007 060729
061201 N Stratta et al. 2007 051016B 060814
061210 051109B 060904B
061217 060505 N Fynbo et al. 2006 061021
070429B 060614 N Fynbo et al. 2006 061028
070714B Della Valle et al. 2006b 061110A
070724A N Kocevski et al. 2010 Gal-Yam et al. 2006 070318
070809 060912 070419A Y Dai et al. 2008
071227 N D’Avanzo et al. 2009 071010A Y Covino et al. 2008 070508
080905A N Rowlinson et al. 2010 080430 070612A
081007 Y Della Valle et al. 2008 071010B
080319B Y Tanvir et al. 2008
Bloom et al. 2009
080710
080916A

0 Yes 8 No 6 No data 5 Yes 3 No 5 No data 3 Yes 0 No 15 No data

Notes. For each group, we present three columns containing the name of the burst, the existence of a detected supernova (Y for yes; N for no; – if the data are not constraining), and references. The last row provides a summary of the total number for each case.

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