petitRADTRANS.pyth_input

Module Contents

Functions

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, border_lambda_angstroem, temp, press, mmw, abundances)

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.

petitRADTRANS.pyth_input.sort_opa_PTgrid(path_ptg)
petitRADTRANS.pyth_input.get_custom_PT_grid(path, mode, species)