Image Details
Caption: Figure 10.
Representative best-fit spectra for ROIs #1, #8, and #13. Each plot shows the NIMS reflectance data (blue points) with 2σ uncertainty (shaded), the combined best-fit model (orange dashed line), and the individual end-member contributions. The 2σ envelope for ROI #13 is missing due to the lack of surrounding pixels since the pixels that include this region are on the edge of the NIMS cube.
© 2026 The Author(s). Published by the American Astronomical Society.