Table 1: Summary of our photometric observations. Magnitudes are referred to the complex afterglow + host. Errors are 1- $\sigma$ . ^*: average of two measurements obtained on Jan. 9.3 and 10.2.
Start UT Exp. time Seeing R magnitude

2003 Jan. 9.7^* 63 min 1.1 $^{\prime\prime}$ $24.48\pm0.18$

2003 Jan. 15.33 15 min 0.8 $^{\prime\prime}$ $25.07\pm0.15$

2003 Feb. 28.02 75 min 0.8 $^{\prime\prime}$ $25.13\pm0.12$

2003 Mar. 9.01 50 min 1.25 $^{\prime\prime}$ $25.35\pm0.17$

**Table 1:** Summary of our photometric observations. Magnitudes are referred to the complex afterglow + host. Errors are 1- $\sigma$ . ^*: average of two measurements obtained on Jan. 9.3 and 10.2.
Start UT	Exp. time	Seeing	R magnitude
2003 Jan. 9.7^*	63 min	1.1 $^{\prime\prime}$	$24.48\pm0.18$
2003 Jan. 15.33	15 min	0.8 $^{\prime\prime}$	$25.07\pm0.15$
2003 Feb. 28.02	75 min	0.8 $^{\prime\prime}$	$25.13\pm0.12$
2003 Mar. 9.01	50 min	1.25 $^{\prime\prime}$	$25.35\pm0.17$

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