I. INTRODUCTION

II. METHODOLOGY  
A. N-body simulations and WL maps  
B. Identifying and replacing dark matter halos  
C. Fitting halo density profiles  
D. Statistics  
E. Monte Carlo parameter estimation contours

III. RESULTS  
B. Cosmological constraints and biases  
C. Bias directions and goodness-of-fit

IV. DISCUSSION  
A. Robustness of the inferred bias  
B. Cosmology from low-bias statistics  
C. The insensitivity of low peaks to baryon cooling

V. SUMMARY AND CONCLUSIONS