Joint machine learning and analytic track reconstruction for X-ray polarimetry with gas pixel detectors

Abstract

We present our study on the reconstruction of photoelectron tracks in gas pixel detectors used for astrophysical X-ray polarimetry. Our work aims to maximize the performance of convolutional neural networks (CNNs) to predict the impact point of incoming X-rays from the image of the photoelectron track. A very high precision in the reconstruction of the impact point position is achieved thanks to the introduction of an artificial sharpening process of the images. We find that providing the CNN-predicted impact point as input to the state-of-the-art analytic analysis improves the modulation factor ($\sim 1\%$ at 3 keV and $\sim 6\%$ at 6 keV) and naturally mitigates a subtle effect appearing in polarization measurements of bright extended sources known as "polarization leakage".

References in corpus (6)

• Analyzing the Data from X-ray Polarimeters with Stokes Parameters
• Design, Construction, and Test of the Gas Pixel Detectors for the IXPE Mission
• A weighted analysis to improve the X-ray polarization sensitivity of IXPE
• HexagDLy - Processing hexagonally sampled data with CNNs in PyTorch
• Towards Optimal Signal Extraction for Imaging X-ray Polarimetry
• Polarisation Leakage due to Errors in Track Reconstruction in Gas Pixel Detectors