1 INTRODUCTION
2 DATA AND SAMPLE SELECTION
2.1 CANDELS/3D-HST Photometry
2.2 MOSDEF Spectroscopy
2.3 Sample Selection
3 METHODOLOGY AND MEASUREMENTS
3.1 Image Smoothing
3.2 SED Fitting
3.3  $E(B-V)_{\text{gas}}$ and SFR Calculations
4 PHOTOMETRIC VS. SPECTROSCOPIC PROPERTIES
4.1 Global vs. Slit Properties
4.2 Difference in $E(B-V)$ vs. SFR
4.3 $\mathbf{H}\alpha$ -to-UV SFR Ratios
4.4 $E(B-V)$ and SFR vs. Size
5 DISCUSSION
5.1 Aperture Effects
5.2 Differences between $E(B-V)_{\text{gas}}$ and $E(B-V)_{\text{stars}}$
5.3 Variations in $\mathbf{H}\alpha$ -to-UV SFR Ratios
6 SUMMARY