with the calculated cooling function
and the
normalization amplitude A.
rsma(1,2,3,4,5,6,7,8,9,10,11,12,13,14)
Note:All abundances are given relative to the "cosmic" abundances. For defaults see [Raymond and Smith1977]. A redshift can be given. This function should be used if single abundances should be fitted. It almost does the same as the model rsmf, only faster. The table exsas_cal:thbrall from the calibration has to be specified under the general key word SPECTRAL_MODEL_FILE of the corresponding spectral parameter file.