models.interpolations#

A subpackage to used to interpolate the KOSMA-\(\tau\) grids and input data and store these methods to use in the evaluation of kosmatau3d. This is a subpackage that can be used for the interpolation of the input data. It will contain functions to interpolate the intensity or optical depth for any species, given an index.

The method of interpolation is passed as an argument when initialising this class. The acceptabled values are ‘linear’, ‘cubic’, and ‘radial’. The default method is ‘linear’. For the large intensity and optical depth grids, ‘cubic’ and ‘radial’ are the same.

Functions

`interpolate_clump_column_density`
`interpolate_clump_dust_intensity`	This will calculate the intensity in Jansky units.
`interpolate_clump_dust_tau`
`interpolate_clump_h2_column_density`
`interpolate_clump_hi_column_density`
`interpolate_clump_species_intensity`	This is converted from brightness temperature to Jansky units.
`interpolate_clump_species_tau`
`interpolate_clump_taufuv`
`interpolate_clump_td`
`interpolate_clump_tg`
`interpolate_fuv`
`interpolate_galaxy_rotation`
`interpolate_h2_mass`
`interpolate_h2_voxel_filling_factor`
`interpolate_hi_mass`
`interpolate_hi_voxel_filling_factor`
`interpolate_interclump_column_density`
`interpolate_interclump_dust_intensity`	This will calculate the intensity in Jansky units.
`interpolate_interclump_dust_tau`
`interpolate_interclump_h2_column_density`
`interpolate_interclump_hi_column_density`
`interpolate_interclump_species_intensity`	This is converted from brightness temperature to Jansky units.
`interpolate_interclump_species_tau`
`interpolate_interclump_taufuv`
`interpolate_interclump_td`
`interpolate_interclump_tg`
`interpolate_number_density`
`interpolate_velocity_dispersion`
`reset`

Modules

models.interpolations.interpolate