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Published on: April 4, 2017
Number of energy windows for photon counting detectors: is more actually more?
1Johns Hopkins University School of Medicine, Radiological Physics Division, The Russell H. Morgan Department of Radiology and Radiological Science, Baltimore, Maryland, United States.
Purpose:
It has been debated whether photon counting detectors (PCDs) with moderate numbers of energy windows ( ) perform better than PCDs with higher . A higher results in fewer photons in each energy window, which degrades the signal-to-noise ratio of each datum. Unlike energy-integrating detectors, PCDs add very little electronic noise to measured counts; however, there exists electronic noise on the pulse train, to which multiple energy thresholds are applied to count photons. The noise may increase the uncertainty of counts within energy windows; however, this effect has not been studied in the context of spectral imaging tasks. We aim to investigate the effect of on the quality of the spectral information in the presence of electronic noise.
Approach:
We obtained the following three types of PCD data with various (= 2 to 24) and noise levels using a Monte Carlo simulation: (A) A PCD with no electronic noise; (B) realistic PCDs with electronic noise added to the pulse train; and (C) hypothetical PCDs with electronic noise added to each energy window's output, similar to energy-integrating detectors. We evaluated the Cramér-Rao lower bound (CRLB) of estimation for the following two spectral imaging tasks: (a) water-bone material decomposition and (b) K-edge imaging.
Results:
For both the e-noise-free and realistic PCDs, the CRLB improved monotonically with increasing for both tasks. In contrast, a moderate provided the best CRLB for the hypothetical PCDs, and the optimal was smaller when electronic noise was larger. Adding one energy window to the minimum necessary for a given task gained 66.2% to 68.7% of the improvement provided.
Conclusion:
For realistic PCDs, the quality of the spectral information monotonically improves with increasing .

