1. INTRODUCTION  
2. THE SCEXAO/CHARIS HIGH-CONTRAST IMAGING PLATFORM  
3. SCEXAO/CHARIS AND KECK/NIRC2 HIGH-CONTRAST SENSITIVITY TO PLANETS AS A FUNCTION OF AGE  
4. TARGET SELECTION  
5. DISCOVERIES FROM THE FIRST FULL YEAR OF THE HGCA SURVEY  
6. DYNAMICAL MASSES  
7. FUTURE DIRECTIONS  