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Table 7.

Results of detailed modelling calculations.

SGRB Vs n0 D 12+log(N/H) 12+log(O/H) T* U log(F) Hβ Tbb z
km s−1 cm−3 pc 104 K a b K
NGC 4993 100 300 0.3 8. 8.82 9.55 0.05 4000 0.009873
050709 120 250 1 7.25 8.81 4.8 0.06 0.19 3000 0.167
051221a 150 100 0.07 7.11 8.82 8.3 0.007 0.007 0.546
061006 100 100 0.27 7.0 8.82 5.7 0.05 0.006 0.4377
061210 100 300 0.93 6.9 8.80 4.3 0.03 0.167 0.4095
070724 120 250 1 7.25 8.81 4.9 0.013 0.072 0.4571
100206A 100 120 1.7 8.04 8.78 4.4 0.9 0.003 2000 0.4068
100206A N 100 250 1.1 8.25 8.82 3.6 0.6 0.025
100206A C 100 200 1.1 8.04 8.82 4.6 0.6 0.0098
100206A S 120 200 0.7 8.15 8.82 4 0.6 0.0092
130603B OTc 140 120 1.8 7.30 8.82 3.6 0.014 0.014 6000 0.356
130603B OTd 150 130 0.3 7.30 8.80 3.5 0.01 0.016
130603B core 150 130 0.3 7.48 8.80 3.5 0.01 0.016
130603B arm 140 120 0.3 7.7 8.82 3.6 0.014 0.03
130603Be 120 100 1 7.47 8.813 3.8 0.007 0.014

Notes.

(a)

F is in photon cm−2 s−1 eV−1 at the Lyman limit;

(b)

in erg cm−2 s−1 calculated at the nebula;

(c)

X-shooter;

(d)

FORS;

(e)

DEIMOS.

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