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 A.1

Continuum opacity data sources.

Ion	Process	Reference
H⁻	b-f	Doughty et al. (1966)
H⁻	f-f	Doughty & Fraser (1966)
H_I	b-f, f-f	Karzas & Latter (1961)
H_I+H_I	CIA	Doyle (1968)
$H_{2}^{-}$ ${\rm{H}}_2^ -$	f-f	Somerville (1964)
$H_{2}^{+}$ ${\rm{H}}_{\rm{2}}^{\rm{ + }}$	f-f	Mihalas (1965)
He⁻	f-f	Somerville (1965), John (1967)
He_I	f-f	Peach (1970)
C_I	f-f	Peach (1970)
Mg_I	f-f	Peach (1970)
Al_I	f-f	Peach (1970)
Si_I	f-f	Peach (1970)
e⁻	scattering	Mihalas (1978)
H₂	scattering	Dalgarno & Williams (1962)

Notes. Bound-free processes are denoted by b-f. Free-free processes are denoted by f-f. Collision induced absorption processes are denoted by CIA.

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