Table 1: Magnitudes for the local sequence stars in the field of SN 2003du. The stars are identified in Fig. 1.
ID U B V R I
1   $13.80\pm 0.01$   $13.81\pm 0.02$   $13.19\pm 0.01$   $12.80\pm 0.003$   $12.43\pm 0.003$
2   $18.34\pm 0.01$   $17.67\pm 0.01$   $16.30\pm 0.01$   $15.31\pm 0.02$   $14.19\pm 0.02$
3   $13.85\pm 0.01$   $13.92\pm 0.02$   $13.37\pm 0.01$   $13.03\pm 0.01$   $12.72 \pm 0.01$
4   $17.76\pm 0.02$   $18.04\pm 0.02$   $17.57\pm 0.01$   $17.22\pm 0.003$   $16.90\pm 0.02$
5   $16.53\pm 0.01$   $16.32\pm 0.03$   $15.58\pm 0.02$   $15.15\pm 0.01$   $14.74\pm 0.01$
6   $18.25\pm 0.04$   $18.67\pm 0.01$   $18.20\pm 0.01$   $17.86\pm 0.01$   $17.50\pm 0.01$
7   $17.14\pm 0.02$   $17.05\pm 0.02$   $16.33\pm 0.02$   $15.91\pm 0.01$   $15.51\pm 0.01$


Source LaTeX | All tables | In the text