Calculation Pluto's surface composition map with modeling temperature IR spectrum of New Horizons LEISA data

Data accompany the paper "Calculation Pluto’s surface composition map with modeling temperature IR spectrum of New Horizons LEISA data" The data contains the results of materials distribution calculation, and some additional data used in the calculations 'Map fits.rar' - archive with map projections of Leisa fits data. Each Leisa measure folder contain 5 fits: 'map_IF.fits' - map of measured reflection coefficients 'map_IF_err.fits' - map of measurements error 'map_emission.fits' - map of radiation emission angles 'map_incidence.fits' - map of radiation incidence angles 'map_phase.fits' - map of phase angles Each map in 'Map fits.rar' is presented for each Leisa band with wavelength in 'bands.fits' 'Data fits.rar' - archive with corrected Leisa data (only measurements in erg/s/cm^2/A/str) and suplying by new flat field in 'flat_field_corr.fits' Further, here fits files with calculated parameters (ice distributions, particle diameters, CH4 solibility in N2, temperature) and files with Scale and Offset (Sj, Oj from paper) parameters for each of 5 Leisa fits: 'params_ls.fits' - Levenberg-Marquard calculations with least square minimization (Sj, Oj in SO_ls.fits) 'params_x2.fits' - Levenberg-Marquard calculations with χ2 - minimization (Sj, Oj in SO_x2.fits) 'params_ls_k1e-9.fits' - calculations with least square minimization and N2 imaginary part of refraction coefficient for λ < 2.1 μm: k = 1e-9 (Sj, Oj in SO_ls_k1e-9.fits) 'params_ls_kmin.fits' - calculations with least square minimization and N2 imaginary part of refraction coefficient for λ < 2.1 μm: k = k(λ0), λ0 = min{ λ: k(λ) > 0} (Sj, Oj in SO_ls_kmin.fits)