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The time and frequency standard system for FAST receivers 被引量:1

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摘要 This paper reports on the time and frequency standard system for the Five-hundred meter Aperture Spherical radio Telescope(FAST),including the system design,stability measurements and pulsar timing observations.The stability and drift rate of the frequency standard are calculated using 1-year monitoring data.The UTC-NIM Disciplined Oscillator(NIMDO)system improves the system time accuracy and stability to the level of 5 ns.Pulsar timing observations were carried out for several months.The weighted RMS of timing residuals reaches the level of less than 3.0μs.
作者 Kai Zhu Jin Fan Kun Liang Wei Tang Zhi-Sheng Gao Yan Zhu Yi Feng Wei-Wei Zhu Lei Qian You-Ling Yue Jin-You Song Xiang-Wei Shi Xing-Yi Wang Ming-Lei Guo Hang Zhang Heng-Qian Gan Hong-Fei Liu Cheng-Jin Jin Peng Jiang 朱凯;范瑾;Kun Liang;Wei Tang;Zhi-Sheng Gao;Yan Zhu;Yi Feng;Wei-Wei Zhu;Lei Qian;You-Ling Yue;Jin-You Song;Xiang-Wei Shi;Xing-Yi Wang;Ming-Lei Guo;Hang Zhang;Heng-Qian Gan;Hong-Fei Liu;Cheng-Jin Jin;Peng Jiang(National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100101,China;National Institute of Metrology,Beijing 100013,China)
出处 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2020年第5期148-154,共7页 天文和天体物理学研究(英文版)
基金 supported by the Joint Research Fund in Astronomy(Grant Nos.U1931129,U1631115 and U1831117)under cooperative agreement between NSFC and Chinese Academy of Sciences(CAS) NSFC-STINT Grant 11611130023(CH2015-6360) the National Natural Science Foundation of China(NSFC,Grant No.11403054)
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