根据《SAGES出版政策》，请您务必在文章中正确采用SAGES出版物标准致谢，具体内容如下: According to the "SAGES Publication Policy", please be sure to correctly use the SAGES publication standards in the article, the details are as follows: SAGES多波段测光巡天是由中国科学院国家天文台天体丰度与星系演化团组负责运行和管理。 The Stellar Abundance and Galactic Evolution Survey (SAGES) is a multi-band photometric project built and managed by the Research Group of the Stellar Abundance and Galactic Evolution of the National Astronomical Observatories, Chinese Academy of Sciences (NAOC). 2、如果您的文章使用了SAGES项目数据，强烈建议您在文中引用以下文章: If your article uses SAGES project data, it is strongly recommended that you cite the following article: [1] The Stellar Abundances and Galactic Evolution Survey (SAGES) -- -- I. General Description and the First Data Release (DR1) , Fan et al. 2023, ApJS, 268, 9 [2] SAGE巡天介绍I: 测光系统和数据处理, 范舟等，天文学进展，2018年，02期，101 [3] SAGE巡天介绍 II：恒星大气参数估计, 赵景昆等，天文学进展，2020年，01期，60-68 [4] The SAGE Photometric Sky Survey: Technical Description, Zheng et al. 2018, RAA,18,147 [5] The Test Area of the SAGE Survey: Zheng et al. 2019, RAA,19,3 [6] The Stellar Abundances and Galactic Evolution Survey: Photonic Passbands and Extinction Coefficients for the u and v Bands, Tan, Ke-Feng et al. 2022, RAA, 22, 10, 105004 [7] Beyond Spectroscopy. II. Stellar Parameters for over 20 Million Stars in the Northern Sky from SAGES DR1 and Gaia DR3, Huang et al. 2023, ApJ, 957, 65 [8] The Stellar Abundances and Galactic Evolution Survey (SAGES) III ---- Data Release 1s NOWT g/r/i-band Data