Table 1: Data from the observations of all long-duration GRBs observed with Chandra or XMM-Newton that place the lowest limit available on the flux.
GRB Obser- $t_{\rm burst}$ Range Flux z Luminosity[1]
  vatory (days) (keV) (10-15 erg cm-2 s-1) (1044 erg s-1)
040223 N 0.75 2-10 170[2] - -
040106 N 0.72 2-10 400[3] - -
031220 C 19 2-10 <3[4] - -
031203 C 50 2-10 4[5] 0.1055[6] 0.099
030723 C 14 0.5-8 <0.5[7] - -
030528 C 12 2-10 4.9[8] - -
030329 N 258 0.5-2 0.6[9] 0.1685[10] 0.041
030328 C 0.64 0.5-3 190[11] 1.52[12] 2434
030227 N 0.81 0.2-10 400[13] 1.6[13] 5818
030226 C 1.5 2-10 32[14] 1.986[15] 791
021004 C 52 2-10 0.7[16] 2.33[17] 25.6
020813 C 43 0.6-6 1450[18] 1.255[19] 11571
020427 C 17 2-10 19[20] - -
020405 C 1.7 0.2-10 1360[21] 0.691[22] 2490
020322 N 0.86 0.2-10 320[23] - -
020321 C 9.9 2-10 <4[24] - -
020127 C 14.3 2-10 26[25] - -
011211 N 0.81 0.2-10 80[26] 2.140[27] 2375
011130 C 82 2-10 <21[28] - -
011030 C 30 2-10 7 - -
010222 C 8.7 2-10 72[29] 1.477[30] 859
010220 N 0.87 0.2-10 33[31] - -
001025A N 910 0.3-12 <4[32] - -
000926 C 13 1.5-8 3.6[33] 2.0379[34] 94.9
000210 C 0.93 2-10 180[35] 0.846[35] 542
991216 C 1.6 2-10 2300[36] 1.02[37] 10990
980425 C 1281 2-10 13[38] 0.0085[39] 0.0018
[1] No bandpass or k-corrections applied; [2] Tiengo et al. (2004a); [3] Reeves & Watson (2004); [4] assuming source #1 (Gendre et al. 2004); [5] this paper ( $\Gamma=1.7$); [6] Prochaska et al. (2004); [7] Butler et al. (2003b); [8] Butler et al. (2003a); [9] Tiengo et al. (2004b); [10] Hjorth et al. (2003); [11] Butler et al. (2003c); [12] Martini et al. (2003); Rol et al. (2003); [13] Watson et al. (2003); [14] Pedersen et al. (2003); [15] Greiner et al. (2003); [16] Sako & Harrison (2002); [17] Møller et al. (2002); Matheson et al. (2003a); Schaefer et al. (2003); [18] Vanderspek et al. (2002); [19] Barth et al. (2003); [20] Fox (2002b); [21] Mirabal et al. (2003); [22] Price et al. (2003); Masetti et al. (2003); [23] Watson et al. (2002b); [24] see In't Zand et al. (2002); [25] Fox (2002a); [26] Reeves et al. (2002); [27] Holland et al. (2002); [28] no single source found (Butler et al. 2002); [29] Harrison et al. (2001a); [30] Jha et al. (2001); Galama et al. (2003); Masetti et al. (2001); [31] Watson et al. (2002a); [32] Pedersen et al. (2004); [33] Harrison et al. (2001b); [34] Castro et al. (2003); [35] Piro et al. (2002); [36] Piro et al. (2000); [37] Piro et al. (2000); Vreeswijk et al. (1999); [38] Kouveliotou et al. (2004); [39] Galama et al. (1998).

Source LaTeX | All tables | In the text