1 INTRODUCTION
2 SAMPLE SELECTION AND DATA PROCESSING
2.1 Correcting for instrumental leakage
2.2 Correcting for ionospheric Faraday rotation
2.3 Mosaicking
2.4 Rotation Measure synthesis
2.5 Noise estimation
3 SOURCE IDENTIFICATION AND VERIFICATION
3.1 Identifying candidate sources
3.2 Verifying candidate sources
3.3 Error quantification
3.4 Candidate evaluation
3.5 Final measurements
4 RESULTS
5 DISCUSSION
5.1 Source sky density
5.2 Comparison with NVSS rotation measures
5.3 Depolarisation analysis
6 SOURCE CLASSIFICATION
6.1 Morphological classification
6.2 Host properties
6.3 Pulsars
6.4 Large-angular-scale radio sources
7 CONCLUSIONS AND FUTURE PROSPECTS