We are interested in developing a DLP instrument for space flight and planetary exploration. The DLP4500NIR EVM supports observations into the near infrared (out to about 2.5 microns). We are interested in pushing these out further using an alternate detector. What may limit the application is the reflectance of the MEMS mirrors and the spectrometer lens transmission. Can the MEMS mirror surface finish be explained? Also, what type of lenses are used in the spectrometer (e.g., SiO2)?]