1 INTRODUCTION  
2 OBSERVATIONS, SAMPLE SELECTION, & METHODS  
2.1 The MOSDEF Survey  
2.2 SED Fitting and Derived Properties  
2.3 Emission-line Fitting  
2.4 Spectral Stacking  
2.5 SDSS Comparison Sample  
3 RESULTS  
4 DISCUSSION  
4.1 MOSDEF \( z\sim2 \) Star-forming Galaxy Completeness  
4.2 MOSDEF \( z\sim2 \) Observed Sample Completeness  
5 SUMMARY