|
par1 | , line energy in keV |
par2 | , gaussian line width in keV |
par3 | , lorentzian FWHM line width in keV |
Norm | , total photons/cm/s in the line |
Both the gaussian and lorentzian lines are 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