Published October 2019 | Version v1
Journal article

A convolutional neural network approach for reconstructing polarization information of photoelectric X-ray polarimeters

  • 1. RIKEN Nishina Center, 2-1 Hirosawa, Wako, Saitama 351-0198 (Japan)
  • 2. Rock Creek Scientific, 1400 East–West Hwy, Silver Spring, MD, 20910 (United States)
  • 3. NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States)
  • 4. The Hakubi Center for Advanced Research, Kyoto University, Kyoto 606-8302 (Japan)
  • 5. Department of Physics, Faculty of Science and Engineering, Chuo University, 1-13-27 Kasuga, Bunkyo-ku, Tokyo 112-8551 (Japan)
  • 6. University of Iowa, Iowa City, IA, 52242 (United States)
  • 7. Hiroshima Astrophysical Science Center, Hiroshima University, 1-3-1 Kagamiyama, Higashi-Hiroshima, Hiroshima 739-8526 (Japan)
  • 8. Core Research for Energetic Universe, Hiroshima University, 1-3-1, Kagamiyama, Higashi-Hiroshima, Hiroshima 739-8526 (Japan)
  • 9. Department of Physical Science, Hiroshima University, 1-3-1 Kagamiyama, Higashi-Hiroshima, Hiroshima 739-8526 (Japan)

Description

This paper presents a data processing algorithm with machine learning for polarization extraction and event selection applied to photoelectron track images taken with X-ray polarimeters. The method uses a convolutional neural network (CNN) classification to predict the azimuthal angle and 2-D position of the initial photoelectron emission from a 2-D track image projected along the X-ray incident direction. Two CNN models are demonstrated with data sets generated by a Monte Carlo simulation: one has a commonly used loss function calculated by the cross entropy and the other has an additional loss term to penalize nonuniformity for an unpolarized modulation curve based on the H-test, which is used for periodic signal search in X-ray/γ-ray astronomy. The modulation curve calculated by the former model with unpolarized data has several irregular features, which can be canceled out by unfolding the angular response or simulating the detector rotation. On the other hand, the latter model can predict a flat modulation curve with a residual systematic modulation down to 1%. Both models show almost the same modulation factors and position accuracy of less than 2 pixel (or 240μm) for all four test energies of 2.7, 4.5, 6.4, and 8.0 keV. In addition, event selection is performed based on probabilities from the CNN to maximize the polarization sensitivity considering a trade-off between the modulation factor and signal acceptance. The developed method with machine learning improves the polarization sensitivity by 10%–20%, compared to that determined with the image moment method developed previously.

Availability note (English)

Available from http://dx.doi.org/10.1016/j.nima.2019.162389

Additional details

Identifiers

DOI
10.1016/j.nima.2019.162389;
PII
S0168900219309726;

Publishing Information

Journal Title
Nuclear Instruments and Methods in Physics Research. Section A, Accelerators, Spectrometers, Detectors and Associated Equipment
Journal Volume
942
Journal Page Range
vp.
ISSN
0168-9002
CODEN
NIMAER

Optional Information

Copyright
Copyright (c) 2019 Elsevier B.V. All rights reserved.