1 INTRODUCTION  
2 PREVIOUS SURVEYS AND DISCOVERIES  
3 SOURCE SELECTION  
3.1 Supernova remnants and candidate supernova remnants  
3.2 High-mass X-ray binaries  
3.3 Globular clusters  
3.4 Pulsar wind nebulae  
4 OBSERVATIONS  
4.1 Setup  
4.2 Survey sensitivity  
4.3 Search  
5 RESULTS  
5.1 Discoveries  
6 DISCUSSION AND CONCLUSIONS