This archive contains data files that can be used to reproduce Figures 7-10 in the article Wieczorek, M. A. (2018) Strength, depth, and geometry of magnetic sources in the crust of the Moon from localized power spectrum analysis, J. Geophys. Res. Planets. The data files contain the final inversion results for the model using magnetized sills, where the full magnetic field to spherical-harmonic degree 449 was employed. For each localized analysis, the best 6 orthogonal localization windows were used that maximized their power within a spherical cap with an angular radius of 8 degrees and with a spherical-harmonic bandwidth of 58. The analyses were performed at the vertices of a quasi equal-area grid with a spacing corresponding to five degrees of latitude. For these models, the file names start with "sills_449_8_58_5". Each file contains the latitude and longitude (in degrees) of the localization analysis, as well as one other value. FILE DESCRIPTIONS sills_449_8_58_5_minchi2r.dat This file contains the minimum reduced chi2 value of the best-fitting model for each analysis. Uncertainties on the inversion parameters were obtained from Monte Carlo simulations that showed 68.2% and 95.4% of the analyses should have reduced chi2 values less than 2.133 and 4.082, respectively. Where 1-sigma uncertainties could not be calculated (when the best-fitting misfits were above the 1-sigma limits) the limit was set to +/- 999.e99. sills_449_8_58_5_db.dat sills_449_8_58_5_db_1m.dat sills_449_8_58_5_db_1p.dat The best-fitting depths to the bottom of the magnetized region and their +/- 1-sigma limits (1p/1m). sills_449_8_58_5_dt.dat sills_449_8_58_5_dt_1m.dat sills_449_8_58_5_dt_1p.dat The best-fitting depths to the top of the magnetized region and their +/- 1-sigma limits. sills_449_8_58_5_rdisk.dat sills_449_8_58_5_rdisk_1m.dat sills_449_8_58_5_rdisk_1p.dat The best-fitting angular radii (in km) of the magnetized sills and their +/- 1-sigma limits. sills_449_8_58_5_rkm2v2.dat sills_449_8_58_5_rkm2v2_1m.dat sills_449_8_58_5_rkm2v2_1p.dat The best-fitting (N M^2 V^2)^(1/2) values in A m^2 of the magnetized sills and their +/- 1-sigma limits.