A photon of energy fully absorbed in silicon produces on average electron-hole pairs, with variance rather than necessarily a Poisson variance. Thus and Gaussian FWHM is . Representative silicon values eV and give about eV FWHM at keV. read noise in split-event pixels, trapping and gain errors broaden that limit; optical pixel size alone does not specify the energy resolution.[ref]
The ASCA Data Reduction Guide by NASA HEASARC. §4.7, non-uniform CTI and Fano-limited FWHM expression
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