The MSG model for cloudy sub-stellar atmospheres - A grid of self-consistent sub-stellar atmosphere models with microphysical cloud formation

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Table C.1

Dust optical data sources. For details on the wavelength ranges please refer to Table 1 in Kitzmann & Heng (2018).

Condensate	Reference
Al₂O₃ [s]	Begemann et al. (1997)^*t; Koike et al. (1995)^t
CaTiO₃[s]	Posch et al. (2003)^t; Ueda et al. (1998) ^f
Fe[s]	Lynch & Hunter in Palik (1991)^t
Fe₂O₃[s]	A.H.M.J. Triaud^*t
FeO[s]	Henning et al. (1995)^*t
FeS[s]	Pollack et al. (1994)^t; Henning & Mutschke (1997)^t
Mg₂SiO₄[s]	Jäger et al. (2003)^*t
MgSiO₃[s]	Jäger et al. (2003)^*t
MgO[s]	Roessler & Huffman in Palik (1991)^t
SiO[s]	Philipp in Palik (1985)^t
SiO₂ [s]	Henning & Mutschke (1997)^*t; Philipp in Palik (1985)^t
TiO₂ [s]	Zeidler et al. (2011)^t; Posch et al. (2003)^t

Notes. We note we use the amorphous (sol-gel) data for Mg₂ SiO₄ [s] and MgSiO₃ [s], and the amorphous data for SiO₂[s].

^* Data from the Database of Optical Constants for Cosmic Dust, Laboratory Astrophysics Group of the AIU Jena.

^t Data from a printed or digital table.

^f Data from a figure.

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