1 INTRODUCTION

2 OBSERVATIONS
2.1 The BETA observations
2.2 The Parkes observations

3 RESULTS
3.1 Transient detection pipelines
3.2 The Parkes observations

4 DISCUSSION
4.1 The pulsar
4.2 Comparison of the pipelines
4.3 Implications for transient sources
4.4 Implications for pulsar discovery

5 CONCLUSION