Thermal removal from near‐infrared imaging spectroscopy data of the Moon

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Sources and physical processes responsible for OH/H2O in the lunar soil as revealed by the Moon Mineralogy Mapper (M3) (2011, methodology): “The method used by the M(3) team [Clark et al., 2011] is simplistic, although about the best that can be done given the limited M(3) data long‐wavelength spectral coverage.”
Near-infrared spectra of ferrous mineral mixtures and methods for their identification in planetary surface spectra (2014, unknown): “…several efforts toward automation of the MGM and other curve-fitting techniques have been successful (Gendrin et al., 2006; Parente et al., 2011; Clénet et al., 2011), further work is needed to develop a fully automated routine that does not require prior knowledge of the mineralogy of the…”
Measuring moonlight: An overview of the spatial properties, lunar coverage, selenolocation, and related Level 1B products of the Moon Mineralogy Mapper (2011, background): “metric and thermal processing required to derived surface reflectance [Clark et al., 2010].”