113-keV window | 208-keV window | ||||
Crystal | Collimator* | 15% | 20% | 15% | 20% |
3/8″ | HE | 6.8 (3.0%) | 7.5 (3.1%) | 7.0 (6.8%) | 7.2 (6.9%) |
3/8″ | ME | 5.8 (3.3%) | 6.3 (3.5%) | 6.0 (7.8%) | 6.1 (8.0%) |
3/8″ | LEGP | 16.1 (31.8%) | 18.6 (35.4%) | 71.5 (84.7%) | 74.6 (84.9%) |
3/8″ | LEHR | 12.0 (43.5%) | 14.3 (47.9%) | 70.3 (90.4%) | 73.2 (90.5%) |
5/8″ | HE | 6.7 (2.9%) | 7.3 (2.9%) | 9.5 (6.9%) | 9.8 (7.0%) |
5/8″ | ME | 5.7 (3.2%) | 6.2 (3.3%) | 8.1 (7.8%) | 8.3 (7.9%) |
5/8″ | LEGP | 14.1 (22.7%) | 16.0 (26.0%) | 95.1 (84.4%) | 98.6 (84.5%) |
5/8″ | LEHR | 9.9 (32.3%) | 11.4 (36.1%) | 92.9 (90.1%) | 96.6 (90.3%) |
↵* GE Infinia camera.
Fractions of detected counts that are due to collimator scatter and septal penetration are shown in parentheses. Some contribution to 113-keV window comes from events from 208-keV photons Compton-scattered in crystal followed by an escape. This contribution increases with decreasing crystal thickness.