|
par1 | , line energy in keV |
par2 | , FWHM line width in keV |
norm | , photons/cm/s in the line |
The line is truncated at the point that the integrated flux under the line is
within a critical value of the total flux. This critical value can be
changed using xset LINECRITLEVEL. The default critical value is
. Note also that the normalization is defined as the
integral over energies greater than zero since negative energies are unphysical.
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Last modified: Friday, 23-Aug-2024 13:20:40 EDT