Polarimetric evaluation of CdTe-Timepix3 detector module for THOR-SR Compton telescope

• Modulation factor ≈0.6 for 100 % linearly polarized gamma rays within 100–300 keV. • Compton efficiency suggests a boost compared to other pixelated CdTe polarimeters. • Polarimeter with sub-degree sensitivity in polarization angle measurement. • Polarimeter with residual statistical polarization fraction of ≈0.03. • MDP lower than 0.3 for 20-day Crab observations with the Compton telescope. Gamma-ray polarimetry for the sub-MeV to lower-MeV band, an unexplored regime, requires the development of polarimeters that utilize novel space instrumentation with enhanced timing, imaging, and polarimetric capabilities, in addition to a robust spectroscopic response. THOR-SR is an astrophysics technology demonstrator to fly aboard the ESA vehicle Space Rider on a two-month mission. The main instrument is an all-sky Compton telescope composed of four layers, each layer with four modules based on 2.0 mm thick CdTe-Timepix3 detectors. Herein, we evaluate the polarimetric performance of a 2.0 mm thick CdTe-Timepix3 detector with 256 × 256 pixels (55 μm pixel size, 1.98 cm² sensitive area, and featuring the Timepix3 chip). For gamma-ray beams, 100 % linearly polarized with energies within 100−300 keV, we explored a method for reconstructing Compton events based on Compton scattering kinematics. Using a selection process, we examined several empirical factors that influence the statistics in the azimuthal angular distribution of scattered gamma rays. Then, we present the response to unpolarized and polarized gamma rays, including beams with very close polarization angles. Finally, an estimate of the THOR-SR telescope's polarization sensitivity in Crab observations is presented. The features of the CdTe-Timepix3 detector enable its operation as a fine Compton polarimeter, ensuring high modulation factors of ≈0.6 and a significantly greater Compton detection efficiency compared to other 2.0 mm thick pixelated CdTe/CZT polarimeters. The laboratory polarimeter exhibits a sub-degree angular sensitivity, capable of distinguishing polarization angles separated by <1.0°, and reveals a residual statistical polarization fraction of ≈0.03. Minimum detectable polarization <0.3 is foreseen in 20-day Crab observations with the THOR-SR Compton telescope.

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Publication Details

Journal
Astroparticle Physics
Published
2025-09-22
DOI
https://doi.org/10.1016/j.astropartphys.2025.103181
Primary Topic
Advanced Semiconductor Detectors and Materials
Type
article
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article

Polarimetric evaluation of CdTe-Timepix3 detector module for THOR-SR Compton telescope

Astroparticle Physics
Advanced Semiconductor Detectors and Materials
article

Polarimetric evaluation of CdTe-Timepix3 detector module for THOR-SR Compton telescope

article en

Abstract

• Modulation factor ≈0.6 for 100 % linearly polarized gamma rays within 100–300 keV. • Compton efficiency suggests a boost compared to other pixelated CdTe polarimeters. • Polarimeter with sub-degree sensitivity in polarization angle measurement. • Polarimeter with residual statistical polarization fraction of ≈0.03. • MDP lower than 0.3 for 20-day Crab observations with the Compton telescope. Gamma-ray polarimetry for the sub-MeV to lower-MeV band, an unexplored regime, requires the development of polarimeters that utilize novel space instrumentation with enhanced timing, imaging, and polarimetric capabilities, in addition to a robust spectroscopic response. THOR-SR is an astrophysics technology demonstrator to fly aboard the ESA vehicle Space Rider on a two-month mission. The main instrument is an all-sky Compton telescope composed of four layers, each layer with four modules based on 2.0 mm thick CdTe-Timepix3 detectors. Herein, we evaluate the polarimetric performance of a 2.0 mm thick CdTe-Timepix3 detector with 256 × 256 pixels (55 μm pixel size, 1.98 cm² sensitive area, and featuring the Timepix3 chip). For gamma-ray beams, 100 % linearly polarized with energies within 100−300 keV, we explored a method for reconstructing Compton events based on Compton scattering kinematics. Using a selection process, we examined several empirical factors that influence the statistics in the azimuthal angular distribution of scattered gamma rays. Then, we present the response to unpolarized and polarized gamma rays, including beams with very close polarization angles. Finally, an estimate of the THOR-SR telescope's polarization sensitivity in Crab observations is presented. The features of the CdTe-Timepix3 detector enable its operation as a fine Compton polarimeter, ensuring high modulation factors of ≈0.6 and a significantly greater Compton detection efficiency compared to other 2.0 mm thick pixelated CdTe/CZT polarimeters. The laboratory polarimeter exhibits a sub-degree angular sensitivity, capable of distinguishing polarization angles separated by <1.0°, and reveals a residual statistical polarization fraction of ≈0.03. Minimum detectable polarization <0.3 is foreseen in 20-day Crab observations with the THOR-SR Compton telescope.

Astroparticle PhysicsVol. 175
University College Dublin (IE), University of Beira Interior (PT), LIP - Laboratory of Instrumentation and Experimental Particle Physics (PT), Instituto de Telecomunicações (PT), University of Coimbra (PT)
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Advanced Semiconductor Detectors and Materials
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