make_splinter_noise_model¶
- beast.observationmodel.noisemodel.splinter.make_splinter_noise_model(outname, sedgrid, frac_unc=0.1, absflux_a_matrix=None, **kwargs)[source]¶
Splinter noise model assumes that every filter is independent with any other. And assumes a fractional uncertainty at all fluxes. No ASTs are used.
- Parameters:
- outname: str
path and filename into which save the noise model
- sedgrid: SEDGrid instance
sed model grid for everyone of which we will evaluate the model
- frac_unc: float [default = 0.10 (10%)]
fractional flux uncertainy
- absflux_a_matrix: ndarray
absolute calibration a matrix giving the fractional uncertainties including correlated terms (off diagonals) for the splinter model, only the diagonal terms are used
- Returns:
- noisefile: str
noisemodel file name