Table 1: Journal of observations of the GRB 001109 field.
Date UT Telescope Filtre Exposure time Limiting magnitude
      (s) (3$\sigma$)
09.7708-09.8590/11/2000 1.23 CAHA (CCD) R 7 $\times $ 500 20.9*  
09.7847-09.8854/11/2000 1.23 CAHA (CCD) B 3 $\times $ 600 20.3*  
09.7848-09.7961/11/2000 4.20 WHT (INGRID) $K_{\rm S}$ 750 19.9**
09.7968-09.8081/11/2000 4.20 WHT (INGRID) H 750 21.0**
09.8083-09.8128/11/2000 4.20 WHT (INGRID) J 300 21.3**
09.8447-09.8845/11/2000 2.56 NOT (StanCam) I 4 $\times $ 600 22.9   
10.0876-10.1084/11/2000 1.00 USNO (CCD) I 1800 21.0*  
10.7363-10.7883/11/2000 3.50 CAHA (OMEGA Prime) H 10 $\times $ 300 20.5*  
10.7618-10.8417/11/2000 1.23 CAHA (CCD) R 9 $\times $ 500 20.9*  
11.8191-11.8281/11/2000 4.20 WHT (INGRID) H 600 20.7**
11.8292-11.8383/11/2000 4.20 WHT (INGRID) $K_{\rm S}$ 600 19.4**
11.8423-11.8514/11/2000 4.20 WHT (INGRID) J 600 21.4**
13.0560-13.0768/11/2000 1.00 USNO (CCD) I 1800 21.0*  
22.1590-22.1938/11/2000 2.56 NOT (ALFOSC) B 600 23.0   
22.8278-22.8444/11/2000 2.56 NOT (ALFOSC) U 2 $\times $ 600 24.0   
23.8035-22.8194/11/2000 2.56 NOT (ALFOSC) B 2 $\times $ 600 23.5   
26.7576-26.7618/11/2000 3.50 CAHA (MOSCA) R 120 22.0   
27.7514-27.7556/11/2000 3.50 CAHA (MOSCA) R 180 22.3   
22.1590-22.1938/05/2001 4.20 WHT (PF) B 3 $\times $ 900 24.0   
22.1951-22.2079/05/2001 4.20 WHT (PF) V 3 $\times $ 450 23.5   
29.1249-29.1795/05/2001 2.56 NOT (ALFOSC) U 3 $\times $ 1500 23.5   
30.1249-30.1723/05/2001 2.56 NOT (ALFOSC) V 900 + 300 23.5   
31.0468-31.0548/05/2001 2.56 NOT (ALFOSC) V 600 22.0   
18.0361-18.0924/06/2001 4.20 WHT (PF) U 5 $\times $ 900 23.5   
30.0583-30.1361/06/2001 3.50 CAHA (OMEGA Cass) $K^\prime $ 120 $\times $ 60 21.0$^{\dag ~}$
01.0354-01.1181/07/2001 3.50 CAHA (OMEGA Cass) $K^\prime $ 120 $\times $ 60 21.0$^{\dag ~}$
24.8655-24.8828/07/2001 6.05 SAO (SCORPIO) R 3 $\times $ 180 25.5   
14.0524-14.0734/08/2001 2.56 NOT (ALFOSC) R 600 + 900 23.8   
14.9983-15.0223/08/2001 2.56 NOT (ALFOSC) R 2 $\times $ 900 24.0   
16.0571-16.1169/08/2001 2.56 NOT (ALFOSC) B 4 $\times $ 1200 25.0   
16.9835-17.0570/08/2001 2.56 NOT (ALFOSC) U 5 $\times $ 1500 24.1   
17.0148-17.0720/08/2001 2.56 NOT (ALFOSC) V 5 $\times $ 900 24.5   
17.0720-17.1148/08/2001 2.56 NOT (ALFOSC) I 6 $\times $ 600 23.7   
05.9503-06.0220/08/2002 2.20 CAHA (BUSCA) y 6 $\times $ 900 22.5   
*   Greiner et al. (2000).  Their BRI band limiting magnitudes have been shifted to our zero point.
** Vreeswijk et al. (2000).  Their ${\it JHK}_{\rm S}$ band limiting magnitudes have been shifted to our zero point.
$\dagger$   The images from 30/6-01/07/2001 were coadded in just a single limiting magnitude, $K^\prime= 21.0$.

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