Table 4.
Summary of probability distributions of radiation effectiveness factors (REFs) for photons and electrons in IREP.a
| Photonsb | 95% confidence interval of REFLc |
|||
|---|---|---|---|---|
| Energy | Exposure | 2.5th percentile | 50th percentile | 97.5th percentile |
| >250 keVd | All | — | 1.0 | — |
| 30–250 keV | All | 1.0 | 1.9 | 4.7 |
| <30 keV | All | 1.1 | 2.4 | 6.1 |
| Electronse | 95% confidence interval of REFLc |
|||
| Energy | Exposure | 2.5th percentile | 50th percentile | 97.5th percentile |
| >15 keVf | All | — | 1.0 | — |
| <15 keVg | All | 1.2 | 2.4 | 5.0 |
Adapted from Table 15 of Kocher et al. (2005). REFs apply to any cancer type.
Probability distributions are described in Table 11 of Kocher et al. (2005); distributions are not described by commonly used continuous distributions (e.g., lognormal).
REFL is REF at low doses and low dose rates of reference high-energy (>250 keV) photons.
Reference radiation with defined REF of unity.
Probability distributions are described in Table 13 of Kocher et al. (2005); distribution for electrons of energy >15 keV is lognormal.
An REFL for 15–60 keV electrons consistent with REFL for 30-250 keV photons is indicated on theoretical grounds, but is not adopted; see Kocher et al. (2005), Table 13, footnote c.
Auger-emitting radionuclides incorporated into DNA are excluded. Beta particles produced in radioactive decay are included if average energy of continuous spectrum of electrons is < 15 keV.