The Mini-SiTian Array: the Mini-SiTian Real-time Image Processing Pipeline (STRIP)

Abstract This paper provides a comprehensive introduction to the mini-SiTian Real-time Image Processing pipeline (STRIP) and evaluates its operational performance. The STRIP pipeline is specifically designed for real-time alert triggering and light curve generation for transient sources. By applying the STRIP pipeline to both simulated and real observational data of the Mini-SiTian survey, it successfully identified various types of variable sources, including stellar flares, supernovae, variable stars, and asteroids, while meeting requirements of reduction speed within 5 minutes. For the real observational data set, the pipeline detected one flare event, 127 variable stars, and 14 asteroids from three monitored sky regions. Additionally, two data sets were generated: one, a real-bogus training data set comprising 218,818 training samples, and the other, a variable star light curve data set with 421 instances. These data sets will be used to train machine learning algorithms, which are planned for future integration into STRIP.

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Publication Details

Journal
Research in Astronomy and Astrophysics
Published
2025-03-31
DOI
https://doi.org/10.1088/1674-4527/adc790
Citations
9
Primary Topic
3D IC and TSV technologies
Type
article
Field-Weighted Citation Impact
6.57

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The Mini-SiTian Array: the Mini-SiTian Real-time Image Processing Pipeline (STRIP)

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article en
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Abstract

Abstract This paper provides a comprehensive introduction to the mini-SiTian Real-time Image Processing pipeline (STRIP) and evaluates its operational performance. The STRIP pipeline is specifically designed for real-time alert triggering and light curve generation for transient sources. By applying the STRIP pipeline to both simulated and real observational data of the Mini-SiTian survey, it successfully identified various types of variable sources, including stellar flares, supernovae, variable stars, and asteroids, while meeting requirements of reduction speed within 5 minutes. For the real observational data set, the pipeline detected one flare event, 127 variable stars, and 14 asteroids from three monitored sky regions. Additionally, two data sets were generated: one, a real-bogus training data set comprising 218,818 training samples, and the other, a variable star light curve data set with 421 instances. These data sets will be used to train machine learning algorithms, which are planned for future integration into STRIP.

Research in Astronomy and AstrophysicsVol. 25(4)
Chinese Academy of Sciences (CN), National Astronomical Observatories (CN), University of Chinese Academy of Sciences (CN)
National Natural Science Foundation of China, Chinese Academy of Sciences, University of Chinese Academy of Sciences, National Astronomical Observatories, Chinese Academy of Sciences
Openalex Percentile: Top 3%
3D IC and TSV technologies
6.57
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