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Home All issues Volume 495 / No 3 (March I 2009) A&A, 495 3 (2009) 1005-1032 Full HTML
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Table 3:

Results of fitting spectra of INTEGRAL GRBs with a power law model.

#		 Name Peak flux Fluence Photon index $\mathbf{\chi^{2}_{\rm red}}$ d.o.f. T90
    (15-150 keV) (20-200 keV) (power law model)  
    [10-8 erg/cm2 s] [10-8 erg/cm2]       [s]

2		 021219 >28.7 >94.6 $1.69^{\rm -0.08}_{+0.09}$ 1.46 46 5.0
4 030227 7.0 74.9 $1.75^{\rm -0.10}_{+0.11}$ 1.0 46 15.0
5 030320 68.0 1131.9 $1.28^{\rm -0.07}_{+0.07}$ 1.8 24 48.0
6 030501 18.4 282.1 $1.83^{\rm -0.07}_{+0.08}$ 1.5 46 25.0
7 030529 1.1 5.2 $3.50^{\rm -0.43}_{+0.51}$ 1.0 9 16.0
8 031203 12.8 134.8 $1.50^{\rm -0.09}_{+0.09}$ 1.3 46 19.0
9 040106 6.2 105.9 $1.58^{\rm -0.14}_{+0.15}$ 1.1 46 48.0
10 040223 2.1 147.7 $2.11^{\rm -0.16}_{+0.17}$ 0.8 46 198.0
11 040323 17.15 190.4 $1.07^{\rm -0.06}_{+0.07}$ 1.7 46 14.0
12 040403 3.3 28.5 $1.84^{\rm -0.15}_{+0.16}$ 1.0 46 15.0
13 040422 20.7 44.2 $2.01^{\rm -0.08}_{+0.09}$ 1.7 46 4.0
14 040624 4.5 48.1 $2.02^{\rm -0.18}_{+0.20}$ 0.8 46 27.0
15 040730 3.0 57.8 $1.44^{\rm -0.15}_{+0.16}$ 0.8 39 42.0
16 040812 4.55 14.0 $2.20^{\rm -0.21}_{+0.22}$ 0.9 28 8.0
17 040827 6.35 101.0 $1.58^{\rm -0.19}_{+0.21}$ 1.1 15 32.0
18 040903 2.3 9.6 $2.90^{\rm -0.39}_{+0.46}$ 0.5 23 7.0
19 041015 2.3 51.2 $1.13^{\rm -0.18}_{+0.18}$ 1.0 35 30.0
20 041218 22.7 491.9 $1.57^{\rm -0.05}_{+0.05}$ 1.3 46 38.5
21 041219 >130 >2100 1.89 0.01+0.01 1.1 46 239.0 (460)8
22 050129 2.4 41.0 $1.7^{\rm -0.25}_{+0.27}$ 0.7 27 30.0
23 050223 4.0 81.5 $1.64^{\rm -0.22}_{+0.24}$ 1.0 46 30.0
24 050502 12.3 >108.6 $1.51^{\rm -0.05}_{+0.06}$ 1.6 46 >11.0
25 050504 3.8 116.0 $1.20^{\rm -0.09}_{+0.09}$ 1.5 46 44.0
26 050520 8.9 159.9 $1.64^{\rm -0.06}_{+0.07}$ 1.1 46 52.5
27 050522 1.5 6.9 $2.65^{\rm -0.48}_{+0.59}$ 1.0 21 10.8
28 050525 >314.8 >1300.0 $1.93^{\rm -0.05}_{+0.00}$ 1.9 39 9.0
29 050626 2.7 66.5 $2.04^{\rm -0.14}_{+0.15}$ 0.6 39 56.0
30 050714 2.9 42.7 $2.03^{\rm -0.19}_{+0.21}$ 1.0 43 34.0
31 050918 15.3 480.0 $1.77^{\rm -0.09}_{+0.10}$ 0.9 39 280.0
32 050922 1.1 5.9 $1.85^{\rm -0.58}_{+0.69}$ 0.7 11 10.0
33 051105B 3.6 20.4 $1.84^{\rm -0.23}_{+0.26}$ 1.0 46 14.0
34 051211B 7.0 179.0 $1.54^{\rm -0.09}_{+0.10}$ 1.0 39 47.0
35 060114 1.6 98.9 $0.95^{\rm -0.18}_{+0.19}$ 1.1 21 80.0
36 060130 1.9 22.5 $1.59^{\rm -0.31}_{+0.34}$ 1.4 22 19.0
37 060204 1.8 46.8 $1.35^{\rm -0.23}_{+0.24}$ 1.0 25 52.0
38 060428C 30.1 201.0 $1.55^{\rm -0.04}_{+0.05}$ 1.9 46 10.4
39 060901 69.2 564.6 $1.43^{\rm -0.06}_{+0.06}$ 1.1 46 16.0
40 060912B 1.3 69.4 $1.65^{\rm -0.28}_{+0.30}$ 1.2 25 140.0
41 060930 4.9 26.3 $1.51^{\rm -0.27}_{+0.30}$ 1.2 33 9.0
42 061025 9.7 97.5 $1.34^{\rm -0.07}_{+0.08}$ 1.6 46 11.0
43 061122 146.2 459.2 $1.71^{\rm -0.04}_{+0.05}$ 1.6 39 11.9
44 070309 2.6 35.7 $1.36^{\rm -0.30}_{+0.31}$ 1.3 16 22.0
45 070311 8.5 137.9 $1.34^{\rm -0.12}_{+0.13}$ 1.0 46 32.0

8 If we include the precursors, see text.


Source LaTeX | All tables | In the text

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