The modeling was performed for the materials listed in the table below. We considered the wavelengths 0.45 micron (blue filter, the results can be applied to B and G filters) and 0.65 micron, i.e. R (red) filter. The table shows the values of the complex refractive index for both wavelengths and the references where the values have been taken from.
Each reference in the table below is a hyperlink to that paper. The table is reproduced from Ivanova et al. (2019).
| Material | $m$ | $m$ | Reference |
|---|---|---|---|
| Blue Filter | Red Filter | ||
| Halley-like dust | $1.88 + i0.47$ | $1.98 +i0.48$ | Kirmura et al. (2003) |
| Amorphous silicate (forsterite) | $1.689 + i0.0031$ | $1.677 + i0.0044$ | Scott and Duley (1996) |
| Water ice | $1.3157 + i1.54 \times 10^{-9}$ | $1.308 + i1.43 \times 10^{-8}$ | Warren (1984) |
| Carbon dioxide ice | $1.42 + i7.04 \times 10^{-7}$ | $1.41 + i1.05 \times 10^{-6}$ | Warren (1986) |
| Iron-rich pyroxene | $1.702 + i0.0596$ | $1.675 + i0.0212$ | Dorschner et al. (1995) |
| Olivine | $1.777 + i0.126$ | $1.743 + i0.066$ | Dorschner et al. (1995) |
| Amorphous carbon | $1.95 + i0.786$ | $2.14 + i0.805$ | Rouleau and Martin (1991) |
| Pyrrhotite (FeS) | $1.45 + i1.53$ | $1.70 + i1.86$ | Egan and Hilgeman (1977) |
| Iron-rich olivine (fayalite) | $1.85 + i0.0015$ | $1.85 + i0.00077$ | Fabian et al (2001) |
| Cosmic organic refractory | $1.9146 + i0.3173$ | $1.98 +i0.2677$ | Li and Greenberg (1997) |
| Tholin ice | $1.56 + i0.0025$ | $1.540 + i0.0012$ | Khare et al. (2003) |
| Titan tholins | $1.58 + i0.0058$ | $1.557 +i0.0009$ | Ramirez et al. (2002) |