I. INTRODUCTION

II. METHOD
A. Scale-dependent halo bias
B. Fisher matrix forecasts
C. From halos to galaxies

III. DEPENDENCE OF SENSITIVITY TO fNL ON SURVEY PROPERTIES
A. Survey depth (minimum stellar mass M*,min)
B. Stellar mass scatter σlog M*
C. Survey volume
D. Maximum wave vector and redshift accuracy
E. Summary and discussion of survey optimization

IV. PUTTING IT ALL TOGETHER: INCLUDING REDSHIFT DEPENDENCE OF THE GALAXY SAMPLE
A. A toy model for an fNL galaxy survey
B. Upcoming/proposed surveys

V. CONCLUSIONS