sesamme.models

Functions

apply_ext_law(x, ebv, y_model)	Redden a model spectrum for comparison with the data.
get_mask(windowlist, x)	Define one or more subsets of wavelength space to ignore when performing the data-model comparison (e.g., sky or geocoronal lines, ISM features).
get_model(theta, x, model_cube, ion_table[, ...])	Construct a model star cluster spectrum with values of metallicity, age, extinction, and normalization randomly chosen (within bounds).
load_ionization_table(file_name)	Loads in the table of ionizing photon outputs per SSP associated with a model cube.
load_ssp_cube(file_name)	Loads in the SSP model cube.
nebular_continuum(x, theta, ion_table)	Python equivalent of the Starburst99 function CONTINUUM, for computing the approximate nebular continuum.
set_ext_law(ext_curve)	Sets the curve used to extinguish model spectra.