Development of a MAPS-based Silicon Pixel Beam Telescope

16 Nov 2025, 17:00
10m
2F, Activities Center (Academia Sinica)

2F, Activities Center

Academia Sinica

128 Section 2, Academia Road, Nankang, Taipei 115201, Taiwan
POSTER Detector Concepts, Simulations ALL Poster

Speaker

Lankun Li (IHEP)

Description

To advance particle detector research, a MAPS-based silicon pixel beam telescope has been developed, which will be used in the High-Energy Proton Beam Experimental Station (HPES). As part of the CSNS-Ⅱ upgrade project, HPES will provide a single-particle proton beam with adjustable energy ranging from 0.8 to 1.6 GeV. As the core detector system of HPES, the telescope comprises six ultra-thin telescope modules, each consisting of a Monolithic Active Pixel Sensor (MAPS), an auxiliary PCB board and an aluminum shield box with a cooling system. The material budget per module is about 0.061%X0, equivalent to 50 μm silicon and two layers of shield film with a thickness of 12.5 μm. Simulations indicate that the beam telescope can achieve a telescope resolution better than 2 μm using a 1.6 GeV proton beam. Additionally, an electronics system has been developed for the telescope, with each module equipped with a readout board for individual control. To accommodate DUTs with various sizes, a dedicated high-precision experimental station is available for the users, featuring two telescope arms for mounting the six telescope modules and a six-axis motion stage for the DUTs in the center. The system also includes a trigger detector and a trigger logic unit to provide proton-level trigger signals for both the telescope and the DUT. To validate the design, a prototype with six modules was tested using a 1.3 GeV electron beam. The results demonstrated a spatial resolution of 5.7 μm for the DUT and 2.7 μm for the telescope, with a detection efficiency exceeding 99.5%. Since the beam tests were performed with an electron beam at an energy lower than 1.6 GeV, the effect of multiple Coulomb scattering was more significant, resulting in a slightly worse telescope resolution compared to the simulation.

Authors

Lankun Li (IHEP) Prof. Mingyi Dong (IHEP)

Co-authors

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