The 68% and 95% likelihood contours (dark- and light-gray shaded regions, respectively) we derive on the shape of the UV LFs at z ∼ 2 based on our lensed HFF samples and the presented constraints on the LF from blank-field studies. Each panel shows the likelihood contours derived using one of six lensing v4 models as the truth in our forward-modeling procedure (Bouwens et al. 2017b) and then recovering LF results using the median magnification from the other parametric lensing models. The light shaded regions shown here are similar to those in Figure 4. The blank-field constraints are from Bouwens et al. (2021a) and include essentially all HST observations acquired to date over legacy fields.