Database of Optical Constants for Cosmic Dust

Optical Constants of Carbonates

Calcite (CaCO3) (Posch et al. 2007)

CaCO3 (10 K) Spectra Litxt to a 300dpi and a 600dpi image Calcite E || c n-k-Data Calcite E || a,b n-k-Data CaCO3 (100 K) Spectra Litxt to a 300dpi and a 600dpi image Calcite E || c n-k-Data Calcite E || a,b n-k-Data CaCO3 (200 K) Spectra Litxt to a 300dpi and a 600dpi image Calcite E || c n-k-Data Calcite E || a,b n-k-Data CaCO3 (300 K) Spectra Litxt to a 300dpi and a 600dpi image Calcite E || c n-k-Data Calcite E || a,b n-k-Data

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Dolomite (CaMg(CO3)2) (Posch et al. 2007)

CaMg(CO3)2 (10 K) Spectra Litxt to a 300dpi and a 600dpi image Dolomite E || c n-k-Data Dolomite E || a,b n-k-Data CaMg(CO3)2 (100 K) Spectra Litxt to a 300dpi and a 600dpi image Dolomite E || c n-k-Data Dolomite E || a,b n-k-Data CaMg(CO3)2 (200 K) Spectra Litxt to a 300dpi and a 600dpi image Dolomite E || c n-k-Data Dolomite E || a,b n-k-Data CaMg(CO3)2 (300 K) Spectra Litxt to a 300dpi and a 600dpi image Dolomite E || c n-k-Data Dolomite E || a,b n-k-Data

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All n-k-Data tables consist of three columns. The first one contains the wavelength in micron. The second one is the real part of the complex refractive index (n), the third one is the imaginary part (k).

For the details of the derivation of all n-k-Data we refer to the mentioned publications (see the List of Publications).