Table 1: List of observations retrieved from the archives with some basic information (configuration of the instruments, instrument that detected the prompt emission). We also report the first refereed publication on the X-ray afterglow.
GRB  Instrument archive Prompt Fluence (band) Afterglow Redshift Ref.
    Obs-ID detection erg.cm-2 (keV) Detection    
GRB 991216 Chandra ACIS-S, HETG 596 BATSE $2\times10^{-4}$ (20-300) X, opt, rad 1.02 1
GRB 000210 Chandra ACIS-S 602 BeppoSAX $6.1\times10^{-6}$ (40-700) X, rad 0.846 -
GRB 000926 Chandra ACIS-S 598, 1047 Ulysses $2.2\times10^{-5}$ (25-100) X, opt, rad 2.066 2
GRB 010222 Chandra ACIS-S 2424, 1048 BeppoSAX $9.25\times10^{-5}$ (40-700) X, opt, rad 1.477 -
GRB 011030 Chandra ACIS-S 3411, 3412 BeppoSAX $1.13\times10^{-6}$ (40-700) rad <3 -
GRB 011130 Chandra ACIS-I 2823 HETE-2 - - - -
GRB 020127 Chandra ACIS-I 3436, 3437 HETE-2 - X, rad - -
GRB 020321 Chandra ACIS-S 3477 BeppoSAX $3.0\times10^{-6}$ (40-700) - - -
GRB 020405 Chandra ACIS-S, LETG 2825 Ulysses $3\times10^{-5}$ (25-100) X, opt, rad 0.69 15
GRB 020427 Chandra ACIS-S 3493, 3494 BeppoSAX ${<}2.9\times10^{-7}$ (40-700) X - 3
GRB 020531 Chandra ACIS-I 2824, 3673 HETE-2 $1\times10^{-7}$ (8-40) - - -
GRB 020813 Chandra ACIS-S, HETG 4364 HETE-2 $3.8\times10^{-5}$ (25-100) X, opt, rad 1.25 4
GRB 021004 Chandra ACIS-S, HETG 4381, 4409 HETE-2 $3.2\times10^{-6}$ (7-400) X, opt, rad 2.3 4
GRB 021201 Chandra ACIS-I 3784, 3785 IPN $2\times10^{-7}$ (25-100) - - -
GRB 030226 Chandra ACIS-S 4425 HETE-2 $5.7\times10^{-6}$ (30-400) X, opt 1.98 5
GRB 030328 Chandra ACIS-S, LETG 4432 HETE-2 $3.0\times10^{-5}$ (30-400) X, opt 1.52 -
GRB 030528 Chandra ACIS-S 3920, 3921 HETE-2 $4.8\times10^{-6}$ (30-400) X, opt - 6
GRB 030723 Chandra ACIS-S -I 3918, 3922 HETE-2 $0.2\times10^{-7}$ (30-400) X, opt - 18
GRB 031220 Chandra ACIS-I 3905, 3906 HETE-2 $1.9\times10^{-6}$ (25-100) X, opt - 7
GRB 040701 Chandra ACIS-I 4661, 4662 HETE-2 $4.5\times10^{-7}$ (2-25) X 0.2146 -
GRB 040812 Chandra ACIS-S 5364, 5365 INTEGRAL $2.5\times10^{-7}$ (20-200) X - -
GRB 001025A XMM-Newton 0128530301 Ulysses $3.2\times10^{-6}$ (25-100) - - 8
GRB 010220 XMM-Newton 0111520301 BeppoSAX - - - 8
    0111520401          
GRB 011211 XMM-Newton 0094380101 BeppoSAX $3.7\times10^{-6}$ (40-700) X, opt 2.14 9
GRB 020321 XMM-Newton 0008820401 BeppoSAX $3.0\times10^{-6}$ (40-700) - - -
GRB 020322 XMM-Newton 0110980301 BeppoSAX - X, opt - 10
    0128530801          
GRB 030227 XMM-Newton 0128531201 INTEGRAL $8.8\times10^{-7}$ (20-200) X, opt - 11
GRB 030329 XMM-Newton 0128531401 HETE-2 $1\times10^{-4}$ (30-400) X, opt, rad 0.168 12
    0128531501          
    0128531601          
GRB 031203 XMM-Newton 0158160201 INTEGRAL $1.5\times10^{-6}$ (20-200) X, opt, rad 0.105 13
    0163360201          
GRB 040106 XMM-Newton 0158160401 INTEGRAL $8.3\times10^{-7}$ (20-200) X, opt - 14
GRB 040223 XMM-Newton 0158160601 INTEGRAL $4.4\times10^{-7}$ (20-200) X - 17
GRB 040827 XMM-Newton 0164570401 INTEGRAL - X, opt - 16
N.B. References are: 1: Piro et al. (2000), 2: Piro et al. (2001), 3: Amati et al. (2004), 4: Butler et al. (2003), 5: Klose et al. (2004), 6: Rau et al. (2004), 7: Melandri et al. (2006), 8: Watson et al. (2002a), 9: Reeves et al. (2002), 10: Watson et al. (2002b), 11: Mereghetti et al. (2003), 12: Tiengo et al. (2003), 13: Watson et al. (2004), 14: Gendre et al. (2004a), 15: Mirabal et al. (2003), 16: De Luca et al. (2005), 17: McGlynn et al. (2005), 18: Butler et al. (2005).

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