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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 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 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(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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