Impact of the ADC Nonlinearities on X-ray Spectral Analysis and Correction Techniques

箱子 线性 动态范围 质心 物理 噪音(视频) 像素 积分非线性 谱线 光学 算法 数学 计算机科学 功率(物理) 人工智能 转换器 量子力学 天文 图像(数学)
作者
A. Castoldi,M. Ghisetti,C. Guazzoni,Cyril Danilevski,D. Lomidze,M. Porro
标识
DOI:10.1109/nssmicrtsd49126.2023.10338469
摘要

Analog-to-digital conversion (ADC) is a key element in spectroscopic systems with low-noise and high dynamic range and the impact of ADC non-linearities must be carefully estimated. Aim of this work is to study the impact of the ADC non-linearity errors and the benefit of suitable correction to experimental X-ray spectra. A simulative study was first conducted on the impact on centroid determination and on the discrimination of two X-ray lines. Correction techniques were applied to experimental X-ray spectra acquired by a ladder (512 x 128 pixels) of the Mini-SDD X-ray imager, featuring a fast 8-bit ADC integrated in the hexagonal pixel (136 μm side) and noise performance down to 40 electrons rms. We measured the individual ADC bin-edges with the 13-bit DAC available at the periphery of the readout ASIC. Fitting the ADC output vs. the DAC code with multiple error-function model returns the bin edges, the sigma of the bin transitions and the goodness-of-fit parameters. The global ADC staircase showed a relative bin-width non-uniformity (mostly differential non-linearity, DNL) in the range 10-50%. The relative bin-width non-uniformity across a full-size sensor (256 x 128) was found about 10% rms in the periphery of the sensor and 3-4 times larger in the internal rows. This spatial pattern had been already observed, e.g. in gain and noise measurements, confirming the relevance of DNL errors.X-ray spectra of Cu target have been compared before and after correction of the ADC bin widths. Both the pedestal and Cu Ka peak as well as the low-energy continuum visually recover a smoother trend. The root-mean-square error (RMSE) of the Cu Ka peak fit shows a marked reduction by a factor 3 after DNL correction. This is also reflected in the marked drop from 4% to 0.5% of the standard error of gain, directly linked to the improved peak fitting, which shows the significant benefit of the correction.
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