摘要
We present a pulsar candidate identification and confirmation procedure based on a position-switch mode during the pulsar search observations.This method enables the simultaneous search and confirmation of a pulsar in a single observation,by utilizing the different spatial features of a pulsar signal and radio frequency interference(RFI).Based on this method,we performed test pulsar search observations in globular clusters M3,M15 and M92.We discovered and confirmed a new pulsar,M3 F,and detected the known pulsars M3 B,M15 A to G(except C) and M92 A.
作者
Lei Qian
Zhi-Chen Pan
钱磊;潘之辰(National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100101,China;CAS Key Laboratory of FAST,National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100101,China;University of Chinese Academy of Sciences,Beijing 100049,China)
基金
supported by the National SKA Program of China No.2020SKA0120100
supported by the Youth Innovation Promotion Association of CAS (id.2018075)
supported by the Basic Science Center Project of the National Natural Science Foundation of China (Grant No.11703047)
supported by the CAS “Light of West China” Program。