2 SUMMARY OF RELEVANT WEAK LENSING THEORY

3 THE CLUSTER SAMPLE

4 DATA AND DATA REDUCTION

5 WEAK LENSING GALAXY SHAPES

6 CLUSTER MEMBER REMOVAL AND ESTIMATION OF THE SOURCE REDSHIFT DISTRIBUTION

7 WEAK LENSING CONSTRAINTS AND MASS ANALYSIS

8 CONSTRAINTS ON THE M – I_X SCALING RELATION

9 DISCUSSION

10 CONCLUSIONS