`petitRADTRANS.pyth_input`

Module Contents

`sigma_hm_ff`(lambda_angstroem, temp, P_e)	Returns the H- free-free cross-section in units of cm^2
`sigma_bf_mean`(border_lambda_angstroem)	Returns the H- bound-free cross-section in units of cm^2 per H-, as defined on page 155 of
`hminus_opacity`(lambda_angstroem, ...)	Calc the H- opacity.
`sort_opa_PTgrid`(path_ptg)
`get_custom_PT_grid`(path, mode, species)

petitRADTRANS.pyth_input.sigma_hm_ff(lambda_angstroem, temp, P_e): Returns the H- free-free cross-section in units of cm^2 per H per e- pressure (in cgs), as defined on page 156 of “The Observation and Analysis of Stellar Photospheres” by David F. Gray

petitRADTRANS.pyth_input.sigma_bf_mean(border_lambda_angstroem): Returns the H- bound-free cross-section in units of cm^2 per H-, as defined on page 155 of “The Observation and Analysis of Stellar Photospheres” by David F. Gray

petitRADTRANS.pyth_input.hminus_opacity(lambda_angstroem, border_lambda_angstroem, temp, press, mmw, abundances): Calc the H- opacity.