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THE EGS5 CODE SYSTEM

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Table 2.6: Data sources for generalized treatment of photoelectric-related phenomena in <strong>EGS5</strong>.<br />

Data<br />

Source<br />

K-edge energies Table 2 of Table of Isotopes, Eighth Edition [57]<br />

Probabilities of x-ray emission at K- Table 3 of Table of Isotopes, Eighth Edition<br />

and L-shell absorption<br />

K x-ray energies<br />

Table 7 Table of Isotopes, Eighth Edition<br />

K x-ray emission probabilities<br />

Table 7 Table of Isotopes, Eighth Edition, Adjusted<br />

to experimental data by Salem et al.[144]<br />

L1, L2, and L3 edge energies Table 2 of Table of Isotopes, Eighth Edition<br />

L x-ray energies<br />

Table 7b of Table of Isotopes, Eighth Edition (Storm<br />

and Israel [167] is used if data is not available in [57])<br />

Probability of Coster-Kronig L1- and Table 3 of Table of Isotopes, Eighth Edition<br />

L2-shell absorption<br />

L x-ray emission probabilities<br />

Theoretical data by Scofield[146], adjusted to experimental<br />

data by Salem et al.<br />

Average M edge energies Calculated from sub-shell binding energy in Table 2<br />

of Table of Isotopes, Eighth Edition<br />

Auger electron energies<br />

Calculated neglecting correction term by using atomic<br />

electron binding energy in Table 2 of Table of Isotopes,<br />

Eighth Edition<br />

K-Auger intensities<br />

Z = 12 − 17, Table 1 of Assad[11]<br />

Z > 17 Table 8 of Table of Isotopes, Eighth Edition<br />

L-Auger intensities<br />

Table 2 from McGuire[102]<br />

M0 s(Z), M 1 s(Z), M 2 s(Z) and M 3 s(Z)<br />

PHOTX[131]<br />

125

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