Lunar photometric properties at wavelengths 0.5-1.6 μm acquired by SELENE Spectral Profiler and their dependency on local albedo and latitudinal zones

► We derived lunar photometric correction parameters for wavelengths 0.5-1.6 μm. ► We obtained different parameter sets for three albedo groups. ► The parameters cover solar phase angles between 5° and 85°. ► An additional correction method for high latitude regions was investigated. ► The lunar high latitude regions have bluer spectra than the other regions.