perhaps ditch the FWHM flag, and instead supply an instrument table with:
- wavelength range
- convolution model (prism, R, dL, photometry*)
- convolution metric
- independent scale flag
- independent fudge flag
- others???
then can unpack in a loop (with fudge and scale in arrays for easy set in priors)
Makes it trivial to try different instruments and data combinations
- filters to be read in and stored in array as part of runargs , and number used as conv metric