For simultaneous analysis of ASCA spectra with corrections for energy-dependent telescope scattering. The plasma emission models now use relative Solar abundances as set by the abund command. All absorption models except wabs use the same relative abundances as the plasma emission models as set by the abund command. The bremss, vbremss, and zbremss now have a normalization which is not temperature-dependent. See the example file in the release.
Table models All table models now use a FITS format.
Multiple table models can be used simultaneously. The Raymond-Smith model now runs off a table in the standard table model FITS format. An etable model reads an additive table model type file and then takes the exponential of the negative of the input. The mtable model now defaults to 1 rather than 0 when there is no tabulated model for part of the response energy range. All vectors for a given dataset are plotted in the same colour.