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 – noisemodel file name

Return type:

str