Vis and NIR reflectance spectra of basalts altered in cold (Udokan, Siberia) and hot (Ogaden, Ethiopia) arid environments collected to help interpreting the spectra of the surface of Mars (Gurgurewicz et al. 2009, Gurgurewicz et al. 2015)

NIR and MIR reflectance spectra of several mixtures of ice and organic matter at various temperature and pressure conditions to contribute interpreting the composition of the surface of Pluto and Charon (Mège et al. 2014). This dataset can be also used to determine the composition of aerosols in the atmosphere of Titan (Nna-Mvondo et al. 2013, Chevrier et al. 2015).