1 INTRODUCTION  

2 THE STAR FORMATION REFERENCE SURVEY (SFRS)  

3 K-BAND DATA  

4 THE 2D FIT OF SFRS GALAXIES  

5 BEST-FIT MODEL SELECTION  

6 SEPARATION OF DISK/BULGE COMPONENTS  

7 LUMINOSITY AND MASS FUNCTIONS  

8 DISCUSSION  

9 SUMMARY AND CONCLUSIONS