“…The ASTER sensor acquires earth's surface imagery in the VNIR, SWIR and TIR wavelength regions and has offered a great opportunity of using these datasets for mapping of various lithological units 1,7,26 , minerals 5 , hydrothermal alteration such as propylitic, argillic, phyllic and potassic zone 4,15,16,19 . Various image enhancement techniques such as Principle Component Analysis (PCA), Minimum Noise Fraction (MNF), Band Ratios (BRs), Band Combinations (BCs) and Spectral Indices (SIs) 6,7,18,19,27 ; spectral mapping algorithms such as Spectral Angle Mapper (SAM), Spectral Feature Fitting (SFF), Matched Filter (MF), Constrained Energy Minimization (CEM), Linear Spectral Unmixing (LSU), Mixture Tuned Matched Filter (MTMF) have been well employed on ASTER datasets to obtain the lithological, mineral and hydrothermal alteration maps with reasonable accuracies 5,8,12,[15][16][17]28 . Most of the full and sub-pixel spectral algorithms require target spectra or endmember to detect and classify them, which needs a rigorous procedure of spectral data extraction either from image, laboratory or spectral library 14 .…”