图像数据自动化处理与光变曲线抽取程序OA北大核心CSTPCD

The monitoring of transient sources such as variable stars and extrasolar planets yields a significant volume of imaging data.Timely reduction of the data,producing light curves and triggering transient event are pivotal for advancing research in this field.Focus-ing on a group of meter-class optical telescopes located at the Xinglong Observatory of the National Astronomical Observatories of Chinese Academy of Science,an automatic pipeline to reduce time-series raw images and generating normalized differential photometric light curves named PPCLP is built and introduced in this paper.The program is modular,uni-versal,and easy to use,making it adaptable across various operating systems.Employing an improved differential photometric method,PPCLP achieves a differential photometric accu-racy of 10-3.In addition to its compatibility with equatorial telescopes,PPCLP seamlessly processes field-uncorrected images acquired from altazimuth telescopes.The components,features,and usage of the program are described in detail in this paper.A brief introduction on how to use the program is presented using the data obtained from the 60 CM Telescope at the Xinglong Observatory for the variable star V670 And.Lastly,this paper discusses the limitations of the program and outlines potential avenues for future development.