*.par-file, peak list of i-th interval in
If this file exists at starting time, is will be used as input
for starting parameters. Normally, this entry is generated by TEIL
*.par-file will be used for starting
parameters, OUTPUT[i] will not be used.
You must enlarge EPSILON for bad grain statistic (e.g. 5µ grains and both primary plus secondary soller slits). Otherwise INDEX will fail: EFLECH finds ghost peak multiplets. Such multiplets are caused by errorneous peak shape due to bad grain statistic.