Table 6: Afterglow properties of 54 XRRs/XRFS: X-ray ToO observations (AX), time in days of the start of ToO and satellite which performed the observation, optical afterglow detection (OT), time of the OT detection and observed magnitude, Radio afterglow detection (RT) and host galaxy detection.
Events A X ToO Date[d] and istrument OT Date[d] and mR[m] OT Radio T Host galaxy
XRF 971019 - - - - - -
XRR 971024 - - - - - -
XRR 980128 - - - - - -
XRR 980306 - - - - - -
XRF 981226 Y1 0.3, 7.2 ( ${\it BeppoSAX}$) N2 0.40 m >23 Y3 Y?4
XRF 990520 - - N5 0.74 m>22.5 N 6 -
XRF 990526 - - - - - -
XRF 990704 Y 7 0.3, 7.1 ( ${\it BeppoSAX}$) N 8 0.19 m>22.5 N 9 -
XRR 991106 Y? 10 0.33 ( ${\it BeppoSAX}$) N 11 0.42 m>22 N 12 -
XRF 000206 - - - - - -
XRR 000208 - - - - - -
XRF 000416 - - N13 2.64 m>20.7 - -
XRF 000615 Y14 0.42 ( ${\it BeppoSAX}$) N15 0.18 m>21.5 - -
XRF 010213 - - N 16 1.98 m>22 N 17 -
XRF 010225 - - - - - -
XRR 010326B - - N18 0.5 m>21 - -
XRR 010613 - - - - - -
XRR 010629 - - N 19 0.49 m>20.5 - -
XRR 010921 - - Y20 1.05 $m=19.9\pm0.2$ - Y
  - -   0.92 m>20.5 21 - -
XRF 011019 - - N22 1.07 m>22.5 - -
XRR 011030 Y 23 11, 31.2 ( ${\it Chandra}$) N24 0.30 m>21 Y 25 Y?26
XRR 011103 - - - - - -
XRF 011130 Y 27 10, 83 ( ${\it Chandra}$) Y? 28 6.89 $m=23.0\pm0.1$ Y? 29 Y 30
XRR 011211 Y 31 0.5 ( ${\it XMM-Newton}$) Y 32 0.46 $m=20.41\pm0.04$ - Y 33
XRF 011212 - - Y?34 2.00 $m=23.8\pm0.2$ - -
XRR 020124 - - Y 35 1.51 $m=23.84\pm0.17$ - -
XRR 020127 Y 36 4.1, 14.6 ( ${\it Chandra}$) N 37 0.19 m>19.5 Y 38 Y39
XRF 020317 - - Y? 40 0.76 $m=19.6\pm0.1$ - -
XRR 020410 Y 41 0.83, 2.3 ( ${\it BeppoSAX}$) Y 41 0.26 $m=21.0\pm0.5$ N 42 -
XRF 020427 Y 43 0.46, 2.5 ( ${\it BeppoSAX}$) - - Y? 44 Y? 45
    9.2, 17.2( ${\it Chandra}$)        
XRF 020625 - - N 46 0.44 m>18.2 - -
XRR 020812 - - N 47 0.13 m>19 - -
XRR 020819 - - N 48 0.72 m>21.7 Y 49 Y? 50
XRF 020903 - - Y 51 26.5 $m=18.6\pm0.2$ Y? 52 Y 53
        1.00 m>19.8 54    
XRR 021004 Y55 0.85, 52.3( ${\it Chandra}$) Y56 0.48 $m=18.46\pm0.05$ Y57 Y58
XRF 021021 - - - - - -
XRF 021104 - - N 59 0.12 m>21 - -
XRR 021112 - - N 60 0.08 m>21 N61 -
XRR 021211 - - Y 62 0.85 $m=23.20\pm0.18$ N 63 Y64
XRR 030115 - - N65 0.48 m>21 Y 66 Y67
XRR 030323 - - Y 68 0.35 $m=18.83\pm0.09$ - Y69
XRR 030324 - - N70 0.39 m>21.4 N71 Y?72
XRR 030329 Y73 0.2, 1.3 ( ${\it RXTE}$) Y 74 0.37 $m=14.55\pm0.03$ Y 75 Y76
    37, 61, 258( ${\it XMM-Newton}$)        
XRF 030416 - - N77 1.45 m>15 - -
XRR 030418 - - Y78 6.58 $m=24.9\pm0.4$ - -
XRF 030429 - - Y79 0.37 $m=20.20\pm0.15$ N80 Y81
XRF 030528 Y82 6, 12 ( ${\it Chandra}$) N83 0.002 m>18.7 - Y 84
XRF 030723 Y 85 2.1, 12.7 ( ${\it Chandra}$) Y 86 0.86 $m=21.9\pm0.2$ N87 -
XRR 030725 - - Y88 3.89 $m=21.2\pm0.2$ - -
XRR 030821 - - - - - -
XRF 030823 - - N89 0.78 m>22.5 - -
XRF 030824 - - N90 1.72 m>22.5 - -
XRR 031109B - - - - - -
XRR 031220 Y91 5.6, 28.5 ( ${\it Chandra}$) N92 0.23 m>21 - -
(1): Frontera et al. (2000), (2): Lindgren et al. (1999), (3): Frail (1999a), (4): Holland et al. (2000), (5): Castro-Tirado et al. (1999), (6): Frail et al. (2000), (7): Feroci et al. (2001), (8): Jensen et al. (1999a), (9): Rol et al. (1999), (10): Antonelli et al. (1999), (11): Jensen et al. (1999b), (12): Frail (1999b), (13): Price et al. (2000), (14): Nicastro et al. (2001), (15): Stanek et al. (2000), (16): Zhu (2001), (17): Berger & Frail (2001a), (18): Price et al. (2001a), (19): Anderson et al. (2001), (20): Bloom et al. (2001); Lamb et al. (2001); Price et al. (2001b), (21): Sergeev et al. (2001), (22): Komiyana et al. (2001), (23): Heise et al. (2001), (24): Mohan et al. (2001), (25): Harrison et al. (2001), (26): Bloom et al. (2003a), (27): Ricker et al. (2001); Butler et al. (2002), (28): Garnavich et al. (2001), (29): Berger & Frail (2001b), (30): Garnavich et al. (2001), (31): Piro et al. (2005), (32): Sezynski et al. (2001), (33): Burud et al. (2001), (34): Dullighan et al. (2002), (35): Gorosabel et al. (2002), (36): Fox (2002), (37): Lamb et al. (2002), (38): Rol et al. (2002), (39): Fox et al. (2002), (40): Tomita et al. (2002), (41): Nicastro et al. (2004), (42): Frail et al. (2002), (43): Amati et al. (2004), (44): Wieringa et al. (2002), (45): Castro-Tirado et al. (2002); Bloom et al. (2003a), (46): Burnashev et al. (2002), (47): Kawabata et al. (2002), (48): Piccioni et al. (2002), (49): Henden et al. (2002), (50): Levan et al. (2002a), (51): Stefanon et al. (2002), (52): Berger et al. (2002), (53): Levan (2002b), (54): Price et al. (2002), (55): Sako & Harrison (2002a,b), (56): Sahu et al. (2002), (57): Frail & Berger (2002b), (58): Djorgovski et al. (2002), (59): Fox & Price (2002), (60): Schaefer et al. (2002), (61): Frail & Berger (2002a), (62): McLeod et al. (2002), (63): Berger & Frail (2002), (64): Fruchter et al. (2002), (65): Nysewander et al. (2003), (66): Berger & Frail (2003a), (67): Masetti et al. (2003), (68): Wood-Vasey et al. (2003), (69): Vreeswijk et al. (2004), (70): Rykoff & Smith (2003), (71): Berger & Frail (2003b), (72): Nysewander et al. (2004), (73): Schartel (2003); Tiengo et al. (2003b,2004); Marshall & Swank (2003); Marshall et al. (2003), (74): Bartolini et al. (2003), (75): Berger et al. (2003), (76): Bloom et al. (2003b), (77): Lipunov et al. (2003), (78): Dullighan et al. (2003), (79): Rumyantsev (2003), (80): Berger & Frail (2003c), (81): Khamitov et al. (2003), (82): Butler et al. (2003a), (83): Ayani & Yamaoka (2003), (84): Rau et al. (2004), (85): Butler et al. (2003c,b), (86): Fynbo et al. (2004), (87): Fynbo et al. (2003), (88): Vinter et al. (2003), (89): Fox & Hunt (2003a), (90): Fox & Hunt (2003b), (91): Gendre et al. (2004), (92): Fox et al. (2003).

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