Table 2: GRBs detected by INTEGRAL. The columns refer to (from left to right): GRB; right ascension; declination; T90 duration; peak flux; fluence; photon index; $\chi ^2$/degrees of freedom (d.o.f.); afterglow detections in radio, R, infrared, IR, optical, O and X-ray, X. Peak fluxes, fluences and photon indices are given in the 20-200 keV energy range.
GRB RA Dec T90 Peak flux Fluence Photon index $\chi ^2$ Afterglow
      s $\rm ph~cm^{-2}~s^{-1}$ $\rm erg~cm^{-2}~s^{-1}$ $\rm erg~cm^{-2}$   /d.o.f.  
GRB 0211251 19:47:57 28:23:35 24 22 -- $4.8\times10^{-5}$$^\ast$ -2.2 -- --
GRB 021219 2 18:50:27 31:57:17 5.5 3.7 $3.5\times10^{-7}$ $9.0\times10^{-7}$ $-2.00\pm0.10$ -- R
GRB 030131 3 13:28:21 30:40:43 124 1.9 $1.7\times10^{-7}$ $7.0\times10^{-6}$ Table 3 -- O
GRB 030227 4 04:57:34 20:28:16 33 1.1 $9.6\times10^{-8}$ $7.5\times10^{-7}$ $-1.85\pm0.20$ -- X, O
GRB 030320 5 17:51:36 -25:18:52 48 5.7 $5.4\times10^{-7}$ $1.1\times10^{-5}$ $-1.69\pm0.08$ -- --
GRB 030501 6 19:05:33 06:15:57 40 2.7 $2.5\times10^{-7}$ $3.0\times10^{-6}$ $-1.75\pm0.10$ -- --
GRB 030529 09:40:30 -56:20:31 20 0.4 $3.7\times10^{-8}$ $4.0\times10^{-7}$ $-2.07\pm0.30$ 2.9/5 --
GRB 031203 7 $^{\star}$ 08:02:32 -39:50:47 39 2.6 $2.5\times10^{-7}$ $2.0\times10^{-6}$ $-1.63\pm0.06$ -- X, O, R
GRB 040106 8 11:52:18 -46:47:15 47 0.6 $6.5\times10^{-8}$ $8.2\times10^{-7}$ $-1.72\pm0.15$ -- X, O, R
GRB 040223 9 16:39:31 -41:55:47 258 0.2 $1.6\times10^{-8}$ $4.4\times10^{-7}$ $-2.30\pm0.19$ 20.1/20 X
GRB 040323 13:53:49 -52:20:45 14 1.5 $2.0\times10^{-7}$ $3.0\times10^{-6}$ $-1.44\pm0.18$ 10.6/8 O
GRB 040403 10 07:40:54 68:12:55 21 0.5 $4.3\times10^{-8}$ $5.0\times10^{-7}$ $-1.90\pm0.15$ -- --
GRB 040422 11 18:42:01 01:59:04 4 2.3 $1.8\times10^{-7}$ $3.4\times10^{-7}$ Table 3 -- IR
GRB 040624 12 13:00:08 -03:34:08 62 0.7 $4.0\times10^{-8}$ $7.0\times10^{-6}$ $-2.11\pm0.20$ 28.1/33 --
GRB 040730 15:53:14 -56:28:15 51 0.32 $3.4\times10^{-8}$ $6.6\times10^{-7}$ $-1.44\pm0.14$ 34.3/33 --
GRB 040812 16:26:05 -44:42:32 16 0.7 $5.0\times10^{-8}$ $2.3\times10^{-7}$ $-2.34\pm0.29$ 19.5/26 X, R
GRB 040827 15:17:00 -16:08:21 35 0.42 $6.0\times10^{-8}$ $1.2\times10^{-6}$ $-1.83\pm0.18$ 32.5/29 X, O
XRF 040903 18:03:22 -25:15:23 15 0.23 $2.0\times10^{-8}$ $1.4\times10^{-7}$ $-2.94\pm0.44$ 16.6/20 --
GRB 041015 00:18:37 66:51:37 33 0.17 $4.0\times10^{-8}$ $6.0\times10^{-7}$ $-0.95\pm0.28$ 17.4/21 --
GRB 041218 01:39:06 71:20:05 40 3.19 $2.8\times10^{-7}$ $5.5\times10^{-6}$ Table 3 -- O
GRB 041219a 13 00:24:26 62:50:06 186 33 $3.6\times10^{-6}$ $1.6\times10^{-4}$ Table 3 -- O, R
GRB 050129 16:51:12 -03:04:44 40 0.36 $3.0\times10^{-8}$ $4.5\times10^{-7}$ $-1.91\pm0.31$ 21.6/26 --
GRB 050223$^{\star}$ 18:05:36 -62:28:26 39 0.67 $6.0\times10^{-8}$ $8.2\times10^{-7}$ $-1.84\pm0.25$ 21.3/30 X
GRB 050502a$^{\star}$ 13:29:45 42:40:27 20 1.58 $2.0\times10^{-7}$ $>1.4\times10^{-6}$ Table 3 -- O, IR
GRB 050504 13:24:00 40:41:45 58 0.45 $7.4\times10^{-8}$ $1.3\times10^{-6}$ $-1.32\pm0.10$ 50.8/29 X
GRB 050520 12:50:03 30:27:02 80 0.53 $4.0\times10^{-8}$ $2.4\times10^{-6}$ $-1.61\pm0.07$ 26.1/30 X, R
XRF 050522 13:20:35 24:47:30 17 0.2 $1.3\times10^{-8}$ $7.0\times10^{-8}$ $-2.72\pm0.67$ 16.2/17 --
GRB 050525a$^{\star}$ 18:32:33 26:20:23 12 31.7 $3.1\times10^{-6}$ $2.0\times10^{-5}$ Table 3 -- O, R
GRB 050626 12:26:58 -63:08:03 50 0.27 $2.0\times10^{-8}$ $7.6\times10^{-7}$ $-2.20\pm0.14$ 27.6/30 --
GRB 050714a 02:54:21 69:07:34 34 0.18 $1.5\times10^{-8}$ $4.7\times10^{-7}$ $-2.06\pm0.20$ 21.8/28 --
GRB 050918 17:50:26 -25:24:51 115 1.61 $1.6\times10^{-7}$ $3.1\times10^{-6}$ Table 3 -- --
GRB 050922a 18:04:37 -32:01:24 8 0.01 $5.3\times10^{-9}$ $5.3\times10^{-8}$ $-1.85\pm1.01$ 0.6/2 --
GRB 051105b 00:37:51 -40:28:52 16 0.31 $3.0\times10^{-8}$ $2.9\times10^{-7}$ $-1.83\pm0.23$ 25.7/27 --
GRB 051211b 23:02:45 55:04:44 60 0.6 $6.1\times10^{-8}$ $2.0\times10^{-6}$ $-1.62\pm0.10$ 38.4/28 X, R
GRB 060114 13:01:07 -04:44:53 63 0.31 $3.0\times10^{-8}$ $9.0\times10^{-7}$ $-0.98\pm0.16$ 18.9/30 --
GRB 060130 15:16:54 -36:54:43 29 0.11 $7.7\times10^{-9}$ $2.8\times10^{-7}$ $-1.51\pm0.40$ 27.7/22 --
GRB 060204a 15:28:56 -39:26:38 34 0.16 $2.1\times10^{-8}$ $6.6\times10^{-7}$ $-1.43\pm0.27$ 20.3/26 X
GRB 060428c 14 19:00:52 -09:33:00 12 3.9 $3.6\times10^{-7}$ $2.3\times10^{-6}$ Table 3 -- --
GRB 060901 15 19:08:38 -06:38:22 20 8.6 $9.0\times10^{-7}$ $8.7\times10^{-6}$ Table 3 -- X, O
GRB 060912b 18:04:52 -19:52:50 91 0.08 $8.8\times10^{-9}$ $7.1\times10^{-7}$ $-1.52\pm0.23$ 18.5/33 --
GRB 060930$^\dagger$ 20:18:09 -23:37:31 20 0.3 $2.2\times10^{-8}$ $2.5\times10^{-7}$ -- -- --
GRB 061025 20:03:39 -48:14:39 11 1.14 $1.3\times10^{-7}$ $1.1\times10^{-6}$ Table 3 -- X, O
GRB 061122 20:15:21 15:30:51 11 31.7 $3.1\times10^{-6}$ $2.0\times10^{-5}$ Table 3 -- X, O
GRB 070309 17:34:44 -37:56:40 38 0.13 $1.1\times10^{-8}$ $5.4\times10^{-7}$ $-1.73\pm0.27$ 26.5/26 X?
GRB 070311$^\dagger$ 05:50:10 03:22:29 50 0.9 -- $2.0\times10^{-6}$ -- -- X, O
GRB 070615 02:57:14 -04:24:28 27 0.41 $2.8\times10^{-8}$ $5.0\times10^{-7}$ $-1.62\pm0.28$ 21.9/27 --
GRB 070707 17:51:00 -68:52:52 0.8 1.72 $2.1\times10^{-7}$ $2.1\times10^{-7}$ $-1.19\pm0.14$ 51.2/47 X, O
1 Malaguti et al. (2003), 2 Mereghetti et al. (2003a), 3 Götz et al. (2003), 4 Mereghetti et al. (2003c), 5 von Kienlin et al. (2003a), 6 Beckmann et al. (2003), 7 Sazonov et al. (2004), 8 Moran et al. (2005), 9 McGlynn et al. (2005), 10 Mereghetti et al. (2005), 11 Filliatre et al. (2005), 12 Filliatre et al. (2006), 13 McBreen et al. (2006), 14 Grebenev & Chelovekov (2007), 15 A. von Kienlin (priv. comm.).
$^\ast$ 25-500 keV.
$^{\star}$ GRBs with known redshift; GRB 031203 at z=0.106 (Prochaska et al. 2004); GRB 050223 at z=0.584 (Pellizza et al. 2006); GRB 050502a at z=3.793 (Prochaska et al. 2005); GRB 050525a (Foley et al. 2005) at z=0.606.
$^\dagger$ Data unavailable for GRB 060930 (values taken from Gotz et al. 2006) and GRB 070311 (values taken from Mereghetti et al. 2007).

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