1. Introduction  
2. Sample Selection  
2.1. Morphological Types in the K10/3000 Sample  
2.2. Galaxy Distances  
2.3. 2MASS Magnitudes  
3. Luminosity Function Determination  
4. Results  
5. Discussion  
5.1. Morphological Type Dependence of the K-band Luminosity Function  
5.2. The Hubble Type Dependence of Black Hole Mass Functions  
6. Conclusions