Repository: Lunar mantle composition based on spectral and geologic analysis of Low-Ca pyroxene- and olivine-rich rocks exposed on the lunar surface

(1) The following CSV files contain the latitude and longitude of LCP-rich points for Figure 2 and Figure 14.

LCP_LATLON 930 nm.csv for the case of a critical wavelength of 0.930 µm in Fig. 2.
LCP_LATLON 940 nm.csv for the case of a critical wavelength of 0.940 µm in Fig. 14a.
LCP_LATLON 950 nm.csv for the case of a critical wavelength of 0.950 µm in Fig. 14b.
LCP_LATLON 960 nm.csv for the case of a critical wavelength of 0.960 µm in Fig. 14c.

(2) This repository also contains the original resolution data of the MI parameter map M(i,j) used to produce the figures 6 through 12.
The file names are as follows:

High_Res_MI_Mosaic_site_I-B8.tif for site I-B8 (Figure 6).
High_Res_MI_Mosaic_site_I-A3.tif for site I-A3 (Figure 7).
High_Res_MI_Mosaic_site_I-C6.tif for site I-C6 (Figure 8).
High_Res_MI_Mosaic_site_I-D1.tif for site I-D1 (Figure 9).
High_Res_MI_Mosaic_site_S-A1.tif for site S-A1 (Figure 10).
High_Res_MI_Mosaic_site_S-E1.tif for site S-E1 (Figure 11).
High_Res_MI_Mosaic_site_S-F3.tif for site S-F3 (Figure 12).