Table 3: Luminosity ratio k and stretch factor s for GRB-SNe with known redshift normalized to SN 1998bw before and after correcting for host extinction. In cases where no extinction could be derived, only the non-corrected values are given. In all cases the SN fits were derived in the observer R-band frame. This list is complete up to the end of 2005, with the exception of GRB 040924 (Soderberg et al. 2006). These results supersede those presented in Z05. Differences compared to Z05 are basically due to the inclusion of new observational data or a revision of the used value for the Galactic extinction along the line of sight. Furthermore, note that we use different cosmological parameters than those in Z04 and Z05.
GRB/XRF/SN k s k (corrected)
970228 $ 0.40\pm0.29 $ $ 1.45\pm0.95 $ $\cdots$
990712 $ 0.35\pm0.09 $ $ 0.83\pm0.13 $ $\cdots$
991208 $ 0.93\pm0.25 $ $ 1.12\pm0.20 $ 2.62+1.10-0.65
000911 $ 0.63\pm0.29 $ $ 1.40\pm0.32 $ 0.85+0.44-0.26
010921 $ 0.68\pm0.43 $ $ 0.69\pm0.25 $ 1.85+2.82-0.79
011121/2001ke $ 0.59\pm0.02 $ $ 0.80\pm0.02 $ 0.88+0.08-0.07
020405 $ 0.74\pm0.05 $ $ 0.97\pm0.07 $ 0.90+0.15-0.11
020903 $ 0.62\pm0.09 $ $ 0.92\pm0.08 $ $\cdots$
021211/2002lt $ 0.40\pm0.19 $ $ 0.98\pm0.26 $ $\cdots$
030329/2003dh $ 1.06\pm0.11 $ $ 0.85\pm0.10 $ 1.50+0.19-0.16
031203/2003lw $ 0.67\pm0.05 $ $ 1.09\pm0.07 $ 1.28+0.18-0.16
041006 $ 0.90\pm0.05 $ $ 1.38\pm0.06 $ 1.03+0.22-0.09
050525A/2005nc $ 0.49\pm0.04 $ $ 0.77\pm0.04 $ 0.66+0.10-0.08


Source LaTeX | All tables | In the text