The ROMA database (ROck reflectance for MArtian in situ exploration) provides the reflectance spectra between 0.4 µm and 3-4 µm of various terrestrial, Martian and synthethic samples, as a means to document reference measurements for comparison with spectra measured by visible and near-infrared spectrometers on planetary surfaces, with a focus on Martian analogs.
This project was developped in a joint effort between the LGLTPE/UCBL/OSUL (Lyon, France) and IPAG (Grenoble, France).