&3.2\
B &04:54:13.43& $-$03:00:42.9& 19.4$^*$& 27.3$^*$ & 25.5$^*$ & 24.5$^*$ & 23.6$^*$& 23.2$^*$ & 22.0$^*$& 5.1 &2.6\
B(1$\phi$) & & & 20.1 & 28.4 & 26.7 & 24.8 & 24.4 & 24.1 & 23.1 & 4.7 &3.0\
C &04:54:12.66& $-$03:01:16.3& 18.6$^*$& 26.2$^*$ & 24.6$^*$ & 23.7$^*$ & 22.8$^*$& 22.4$^*$ & 21.6$^*$& 5.1 &3.8\
C(1$\phi$) & & & 19.3 & 27.8 & 26.0 & 24.2 & 23.6 & 23.4 & 22.7 & 4.9 &3.4\
D &04:54:12.33& $-$03:01:15.6& 19.4 & 27.0 & 25.9 & 24.4 & 24.1 & 23.6 & $>$22.3 & 5.0 &$>$2.9\
E &04:54:10.92& $-$03:01:24.5& 19.5 & 27.1 & 26.0 & 25.6 & $>$24.5 & $>$24.6 & $>$22.3 & 6.1 &$>$2.8\
F &04:54:11.22& $-$03:01:22.9& 19.7 & 26.8 & 26.6 & 25.5 & $>$24.5 & 23.8 & 22.1 & 5.8 &2.4\
G &04:54:13.66& $-$03:01:21.9& 20.3 & $>$27.3 & $>$26.7 & $>$26.0 & $>$24.5 & $>$24.6 & $>$22.3 & $>$5.7&2.0\
\
\

SMM J $04541-0302$ is unresolved in the SCUBA map at 65from the cluster center, and lens amplification factor is 2.6 (Chapman et al. 2002a). The flux at 850 $\mu$m is 16.8 mJy, and the constraint on photometric redshift derived from radio index is $z \geq$ 2.2. Since this source is 