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Table B.2.

Results of the spectral analysis.

GRB Time interval Model α1 Ebreak keV α/α2 Epeak keV β Flux 10−7erg s−1 cm−2 ℒ (d.o.f.) Instr.
060510B [127.00,325.00] Band [0.22 − 0.79] 1052(1002) X+B
060814 [77.50,200.00] Band 848(1002) X+B
061121 [62.00,110.00] Band [5.32 − 76.78] 794(1002) X+B
070616 [138.00,615.00] Bandcut 968(1001) X+B
070721B [311.00,361.00] PL [0.09 − 2.60] 721(1004) X+B
080906 [78.00,95.00] PL [0.11 − 0.43] 700(1004) X+B
080928 [197.93,256.30] Band [0.66 − 1.13] 1054(1233) X+B+G
081008 [94.00,193.00] Band [0.28 − 0.74] 900(1002) X+B
090709A [75.00,101.00] Band [1.07 − 12.55] 897(1002) X+B
090715B [53.00,295.00] CPL 909(1003) X+B
100413A [147.00,228.00] PL [0.25 − 2.38] 902(1004) X+B
100619A [80.68,100.13] Band [3.30 − 5.40] 1147(1218) X+B+G
100704A [93.37,197.82] Band 1476(1234) X+B+G
100725B [89.49,229.78] Band 818(1002) X+B
100728A [81.53,158.33] Bandcut 1945(1352) X+B+G
100814A [94.70,180.71] Bandcut 1418(1349) X+B+G
100906A [85.72,125.65] Band 1274(1234) X+B+G
110102A [195.17,290.40] Band [1.29 − 9.90] 949(1002) X+B
110119A [162.56,214.79] Band [0.90 − 2.52] 1238(1233) X+B+G
110205A [160.00,350.00] Band [0.65 − 2.36] 926(1002) X+B
111103B [104.00,127.00] CPL 756(1003) X+B
111123A [106.00,274.00] Bandcut 994(1001) X+B
121123A [193.15,299.65] CPL 1029(1003) X+B
121217A [717.30,767.48] Band [1.20 − 2.97] 1383(1233) X+B+G
130514A [96.00,158.00] Band [0.53 − 1.07] 936(1002) X+B
130606A [117.00,166.00] PL [0.35 − 12.83] 878(1004) X+B
130907A [71.00,87.00] Band [6.87 − 203.28] 919(1002) X+B
140108A [76.76,101.33] CPL 1209(1234) X+B+G
140206A [50.25,100.00] Bandcut 844(1001) X+B
140323A [101.52,122.00] Bandcut 1210(1001) X+B+G
140512A [102.86,158.16] Bandcut 1475(1338) X+B+G
141031A [857.00,893.00] Band [0.25 − 1.15] 934(1002) X+B
150724A [216.00,235.00] CPL 732(1003) X+B
151021A [95.00,128.00] Band 868(1002) X+B

Notes. The table lists the GRB name, the best fit model name (PL = power-law, CPL = cutoff power-law, Band = Band function, Bandcut = Band function with a high energy cutoff), the best fit parameters (cols. 4–8, for a definition see Fig. 1), the average flux, the overall likelihood , and the degrees of freedom (d.o.f.). The last column reports the instruments included in the spectral analysis: X = XRT, B = BAT, G = GBM.

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