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Table B.1

Best-fit parameters for the Type II GRBs fitted with Eq. (B.3).

GRB z T°(s) B (1015 G) P (ms) k E° (1050 erg)

051016B 0.9364 600. 7.0 ± 1.3 11.0 ± 1.0 0.80 ± 0.36 0.07 ± 1.3
051109A 2.346 100. 2.8 ± 0.1 1.5 ± 0.1 0.42 ± 0.06 10.0 ± 1.3
051221 0.5465 100. 4.0 ± 0.0 15.0 ± 0.9 0.52 ± 0.12 0.3 ± 0.2
060502A 1.51 400. 2.2 ± 0.5 2.7 ± 0.4 0.25 ± 0.13 3.0 ± 0.8
060605 3.78 300. 4.0 ± 1.8 2.14 ± 0.2 0.99 ± 0.56 3.0 ± 1.5
070306 1.4959 1000. 1.7 ± 8.9 2.8 ± 0.2 0.99 ± 0.33 1.5 ± 0.5
080707 1.23 100. 5.0 ± 0.8 10.2 ± 0.1 0.99 ± 0.60 0.15 ± 0.36
090529 2.625 1000. 1.2 ± 0.6 2.8 ± 0.1 0.89 ± 0.17 2.0 ± 0.8
090618 0.54 160. 3.0 ± 0.0 2.5 ± 0.0 0.81 ± 0.01 12.0 ± 5.0
090927 1.37 1000. 3.2 ± 0.3 5.1 ± 0.1 0.99 ± 0.12 0.8 ± 1.4
100425A 1.755 700. 4.0 ± 0.7 5.2 ± 0.3 0.51 ± 0.14 0.9 ± 0.8
100621 0.542 250. 3.0 ± 0.0 3.8 ± 0.0 0.70 ± 0.02 4.0 ± 0.3

060526 3.21 100. 3.2 ± 1.3 5.5 ± 1.0 0.70 ± 0.06 1.0 ± 0.6
060714 2.71 60. 5.0 ± 2.0 2.8 ± 0.2 0.43 ± 0.05 10.0 ± 6.0
080310 2.43 400. 6.3 ± 0.8 5.8 ± 1.0 0.80 ± 0.06 4.0 ± 1.2
091029 3.79 100. 1.99 ± 0.6 1.6 ± 0.3 0.32 ± 0.01 1.6 ± 0.4

Notes. z is the redshift, T° the initial time, B the best-fit values for magnetic field, P for NS period, k′ for radiative efficiency and E° for blastwave energy. In the lower panel the same values are listed for a set of GRBs with flares (see also the fit of GRB 060729 and GRB 061121 in Dall’Osso et al. 2011).

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