Last updated: October 16, 2018 Contained in this directory are tabulated rest-frame UV luminosity functions (UV LFs) and observer-frame apparent magnitude functions (AMFs) for galaxy populations between z = 4 - 10 predicted by the Santa Cruz semi-analytic model (SAM) for galaxy formation, released along with the first paper of the Semi-Analytic Forecasts for JWST series (Paper I). The label "Fid" indicates predictions from our fiducial star formation and gas partitioning model, which provides the best match to observational constraints across all redshifts. Alternative models "KS" and "GKBig1" are also provided, see section 2.1 for a detailed description. Predictions including dust attenuation are labeled with "dust", and the ones without dust are labeled "nodust". See section 2.5 in Paper I for a detailed description of how dust is treat in our models. For AMFs, we provide predictions for all eight JWST NIRCam broadband filters: F070W, F090W, F115W, F150W, F200W, F277W, F356W, and F444W. We have selected F200W as our nominal filter (see section 4 for details). For both our fiducial model (GKBig2) and nominal filter (F200W), we provide alternative predictions where we change the SNe feedback slope (alpha_rh; labeled as alp; see section 2.3 for model descriptions and section 3.1 for results). For fiducial predictions, we also provide predictions where the gas depletion time (tau_*,0; labeled as tau) is changed by a factor of two (see section 2.1 for model descriptions and section 3 for results). For more details see Yung et al. 2019 and cite MNRAS 483, 2983 or https://arxiv.org/abs/1803.09761v2