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Correcting Charge Sharing Distortions in Photon Counting Detectors Utilizing a Spatial-Temporal CNN

  • Aaron Smith,
  • James Atlas,
  • Ali Atharifard,
  • Corin Simcock,
  • Sikiru A. Adebileje,
  • Steven D. Alexander,
  • Maya R. Amma,
  • Marzieh Anjomrouz,
  • Fatemeh Asghariomabad,
  • Anthony P. H. Butler,
  • Philip H. Butler,
  • Pierre Carbonez,
  • Claire Chambers,
  • Krishna M. Chapagain,
  • Alexander I. Chernoglazov,
  • Jennifer A. Clark,
  • Frances Colgan,
  • Jonathan S. Crighton,
  • Jérôme Damet,
  • Theodorus Dapamede,
  • Niels J. A. de Ruiter,
  • Devyani Dixit,
  • Robert M. N. Doesburg,
  • Karen Dombroski,
  • Neryda Duncan,
  • Steven P. Gieseg,
  • Joseph L. Healy,
  • Luke Holmes,
  • Kevin Jonker,
  • Tracy Kirkbride,
  • V. B. H. Mandalika,
  • Aysouda Matanaghi,
  • Mahdieh Moghiseh,
  • Manoj Paladugu,
  • David Palmer,
  • Raj K. Panta,
  • Peter Renaud,
  • Yann Sayous,
  • Nanette Schleich,
  • Jereena S. Sheeja,
  • Lieza Vanden Broeke,
  • V. S. Vivek,
  • E. Peter Walker,
  • Manoj Wijesooriya

摘要

Charge sharing induces spectral and spatial distortions on photon counting detectors which must be corrected using methods such as charge summing circuitry. We propose a method of correction using a spatial-temporal convolutional neural network based on the CycN-Net design. We compare our results to an analytical scalar matrix correction and a U-Net. We show improvements in two energy channels set to 50 and 60 keV with a mean absolute percentage error reduced from 4.84% and 7.46% to 3.95% and 5.14%, respectively, when compared to the scalar matrix approach. We analyze the use of time offset projections and the incorporation of the arbitration counter as a prior in the CycN-Net and show their usefulness for accurate predictions. We also examine the effects of masking and the use of the analytical scalar matrix correction as preprocessing steps for the CycN-Net model. Our results show the potential of utilizing a spatial-temporal CNN approach for correcting charge sharing distortions in higher energy ranges.