A New Method for Identifying Contaminating Sources and Locating Target Sources through the Cross-Arm Features of Micro Pore Optics
Yiming Huang, Lian Tao, Jin-Yuan Liao, Shuang-Nan Zhang, St\'ephane Schanne, Bertrand Cordier, Shaolin Xiong, Juan Zhang, Zhengwei Li, Qian-Qing Yin, Xiangyang Wen, Sheng Yang, Min Gao, Donghua Zhao, Xiang Ma, Yue Huang, Liang Zhang, and Liming Song

TL;DR
This paper introduces a novel method utilizing cross-arm features of Micro Pore Optics in space telescopes to improve detection and localization of contaminating and target sources, demonstrated through simulations.
Contribution
The paper presents a new technique based on cross-arm PSF analysis for source identification and localization, enhancing capabilities of MPO-based space instruments.
Findings
Can identify contaminating sources at off-axis angles >8' with 200s exposure
Achieves source positioning accuracy of 6' with single detectors
Using a 16x16 SDD array, can detect sources >2.4' off-axis in 1s with 1 Crab flux
Abstract
The Pathfinder of the Type-A satellites in the Chasing All Transients Constellation Hunters (CATCH) space mission is equipped with Micro-Pore Optics (MPOs) and four single-pixel Silicon Drift Detectors (SDDs). Due to the lack of position resolution in an individual SDD, we propose a new method based on the cross-arms in the point spread function (PSF) of MPOs to enhance the satellite's capability in identifying contaminating sources and locating target sources. By placing one detector on each of the horizontal and vertical cross-arms on the focal plane, we can use the changes in the relative counts on the cross-arms detectors to deduce the location of the source. Simulated observations demonstrate that, for a target source with a flux of 1 Crab and an exposure time of 200 s, the cross-arms detectors can identify contaminating source with the same flux level at an off-axis angle larger…
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Taxonomy
TopicsSpacecraft Design and Technology · Space Satellite Systems and Control · Calibration and Measurement Techniques
