Lei Wang, Xiaoming Zhang, Chunhai Bai, Haiwen Xie, Juan Li, Jiayi Ge, Jianfeng Wang, Xianqun Zeng, Jiantao Sun, Xiaojun Jiang
{"title":"Rapid Automatic Multiple Moving Objects Detection Method Based on Feature Extraction from Images with Non-sidereal Tracking","authors":"Lei Wang, Xiaoming Zhang, Chunhai Bai, Haiwen Xie, Juan Li, Jiayi Ge, Jianfeng Wang, Xianqun Zeng, Jiantao Sun, Xiaojun Jiang","doi":"arxiv-2409.02405","DOIUrl":null,"url":null,"abstract":"Optically observing and monitoring moving objects, both natural and\nartificial, is important to human space security. Non-sidereal tracking can\nimprove the system's limiting magnitude for moving objects, which benefits the\nsurveillance. However, images with non-sidereal tracking include complex\nbackground, as well as objects with different brightness and moving mode,\nposing a significant challenge for accurate multi-object detection in such\nimages, especially in wide field of view (WFOV) telescope images. To achieve a\nhigher detection precision in a higher speed, we proposed a novel object\ndetection method, which combines the source feature extraction and the neural\nnetwork. First, our method extracts object features from optical images such as\ncentroid, shape, and flux. Then it conducts a naive labeling based on those\nfeatures to distinguish moving objects from stars. After balancing the labeled\ndata, we employ it to train a neural network aimed at creating a classification\nmodel for point-like and streak-like objects. Ultimately, based on the neural\nnetwork model's classification outcomes, moving objects whose motion modes\nconsistent with the tracked objects are detected via track association, while\nobjects with different motion modes are detected using morphological\nstatistics. The validation, based on the space objects images captured in\ntarget tracking mode with the 1-meter telescope at Nanshan, Xinjiang\nAstronomical Observatory, demonstrates that our method achieves 94.72%\ndetection accuracy with merely 5.02% false alarm rate, and a processing time of\n0.66s per frame. Consequently, our method can rapidly and accurately detect\nobjects with different motion modes from wide-field images with non-sidereal\ntracking.","PeriodicalId":501163,"journal":{"name":"arXiv - PHYS - Instrumentation and Methods for Astrophysics","volume":"13 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Instrumentation and Methods for Astrophysics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.02405","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
Optically observing and monitoring moving objects, both natural and
artificial, is important to human space security. Non-sidereal tracking can
improve the system's limiting magnitude for moving objects, which benefits the
surveillance. However, images with non-sidereal tracking include complex
background, as well as objects with different brightness and moving mode,
posing a significant challenge for accurate multi-object detection in such
images, especially in wide field of view (WFOV) telescope images. To achieve a
higher detection precision in a higher speed, we proposed a novel object
detection method, which combines the source feature extraction and the neural
network. First, our method extracts object features from optical images such as
centroid, shape, and flux. Then it conducts a naive labeling based on those
features to distinguish moving objects from stars. After balancing the labeled
data, we employ it to train a neural network aimed at creating a classification
model for point-like and streak-like objects. Ultimately, based on the neural
network model's classification outcomes, moving objects whose motion modes
consistent with the tracked objects are detected via track association, while
objects with different motion modes are detected using morphological
statistics. The validation, based on the space objects images captured in
target tracking mode with the 1-meter telescope at Nanshan, Xinjiang
Astronomical Observatory, demonstrates that our method achieves 94.72%
detection accuracy with merely 5.02% false alarm rate, and a processing time of
0.66s per frame. Consequently, our method can rapidly and accurately detect
objects with different motion modes from wide-field images with non-sidereal
tracking.