1 INTRODUCTION  
1.1 X-ray binaries in globular clusters  
1.2 NGC 3201  
1.3 The MAVERIC Survey  

2 DATA AND REDUCTION  
2.1 Catalogue selection  
2.1.1 The MAVERIC Survey  
2.1.2 Optical surveys  
2.2 X-ray data reduction  
2.3 Catalogue cross-matching and source identification  

3 RESULTS  
3.1 Known BHs  
3.2 Sub-subgiants and red stragglers  
3.3 Optical/X-ray sources  
3.4 Interesting radio sources  
3.5 X-ray sources  
3.6 Other radio sources  

4 DISCUSSION  
4.1 Accretion limits on the detached black holes  
4.2 Detectability of the black holes with current and future instruments  
4.3 Population of X-ray sources and encounter rate  
4.4 Evolution of sub-subgiants  

5 CONCLUSIONS