# Dead-time correction for spectroscopic photon counting pixel detectors

**Authors:** Gabriel Blaj

arXiv: 1903.06147 · 2019-11-20

## TL;DR

This paper introduces new analytical models for dead-time correction in spectroscopic photon counting pixel detectors, significantly improving linearity at high count rates without prior calibration, crucial for future high-brilliance light sources.

## Contribution

It presents the first models leveraging actual analog pre-amplifier behavior to accurately linearize photon counting detectors, eliminating the need for calibration in certain configurations.

## Key findings

- Complete dead-time correction without calibration for detectors with two counters per pixel
- Analytical models that improve linearity at high count rates
- A general empirical approach for cases where analytical models are insufficient

## Abstract

Modern photon counting pixel detectors enabled a revolution in applications at synchrotron light sources and beyond in the last decade. One of the limitations of current detectors is reduced counting linearity or even paralysis at high counting rates, due to dead-time which results in photon pile-up. Existing dead-time and pile-up models fail to reproduce the complexity of dead-time effects on photon counting, resulting in empirical calibrations for particular detectors at best, imprecise linearization methods, or no linearization. This problem will increase in the future as many synchrotron light sources plan significant brilliance upgrades and free-electron lasers plan moving to a quasi-continuous operation mode. We present here the first models that use the actual behavior of the analog pre-amplifiers in spectroscopic photon counting pixel detectors with constant current discharge (e.g., Medipix family of detectors) to deduce more accurate analytical models and optimal linearization methods. In particular, for detectors with at least two counters per pixel, we completely eliminate the need of calibration, or previous knowledge of the detector and beam parameters (dead-time, integration time, large sets of synchrotron filling patterns). This is summarized in several models with increasing complexity and accuracy. Finally, we present a general empirical approach applicable to any particular cases where the analytical approach is not sufficiently precise.

## Full text

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## Figures

9 figures with captions in the complete paper: https://tomesphere.com/paper/1903.06147/full.md

## References

45 references — full list in the complete paper: https://tomesphere.com/paper/1903.06147/full.md

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Source: https://tomesphere.com/paper/1903.06147