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Improving Pulsar Candidate Identification with Grid Group Uniform Sampling
Song, Yi-Ning1,2; Chen, Mao-Zheng1,3; Liu, Zhi-Yong1,3
2025-05-01
Source PublicationRESEARCH IN ASTRONOMY AND ASTROPHYSICS
ISSN1674-4527
Volume25Issue:5Pages:055007
Contribution Rank1
AbstractPulsar candidate identification is an indispensable task in pulsar science. Based on the characteristics of imbalanced and diverse pulsar data sets, and the lack of a unified processing framework, we first used dimensionality reduction and visualization to analyze potential deficiencies caused by the incompleteness of current data set extraction methods. We found that the limited use of non-pulsar data may lead to bias in the result, which may limit the generalization ability. Based on the dimensionality reduction results, we propose a Grid Group Uniform Sampling (GGUS) method. This data preprocessing method improves the performance of Random Forest, Support Vector Machine, Convolutional Neural Network, and ResNet50 models on Lyon's features, diagnostic plots, and period-dispersion measure (period-DM) plots in the HTRU1 data set. The average recall increased by approximately 0.5%, precision by nearly 2%, and F-1 score by around 1.2% for all models and in all data sets. In the period-DM plots testing, the high-performance ResNet50 algorithm achieved over 98% F-1 using random sampling. GGUS demonstrated further improvements in this test, enhancing the average F-1 score, precision, and recall by approximately 0.07%, 0.1%, and 0.03%, respectively.
Keyword(stars:) pulsars: general methods: data analysis methods: statistical
DOI10.1088/1674-4527/adc85b
Indexed BySCI
Language英语
WOS KeywordCLASSIFICATION ; SELECTION
Funding ProjectNational Key Research and Development Program of China[2018YFA0404603] ; Operation, Maintenance and Upgrading Fund for Astronomical Telescopes and Facility Instruments ; Ministry of Finance of China (MOF)
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:001485160500001
PublisherIOP Publishing Ltd
Funding OrganizationNational Key Research and Development Program of China ; Operation, Maintenance and Upgrading Fund for Astronomical Telescopes and Facility Instruments ; Ministry of Finance of China (MOF)
Citation statistics
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/7740
Collection射电天文研究室_微波技术实验室
Corresponding AuthorChen, Mao-Zheng; Liu, Zhi-Yong
Affiliation1.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China
2.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
3.Chinese Acad Sci, Key Lab Radio Astron & Technol, Beijing 100101, Peoples R China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Song, Yi-Ning,Chen, Mao-Zheng,Liu, Zhi-Yong. Improving Pulsar Candidate Identification with Grid Group Uniform Sampling[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2025,25(5):055007.
APA Song, Yi-Ning,Chen, Mao-Zheng,&Liu, Zhi-Yong.(2025).Improving Pulsar Candidate Identification with Grid Group Uniform Sampling.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,25(5),055007.
MLA Song, Yi-Ning,et al."Improving Pulsar Candidate Identification with Grid Group Uniform Sampling".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 25.5(2025):055007.
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