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X-Ray Pulsar Data Processing and Analysis
- YANG Chengwei1, ZHENG Jianhua2,3
Author information
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1. Mechatronical School,Beijing Institute of Technology,Beijing 100086,China;
2. National Space Science Center,Chinese Academy of Sciences,Beijing 100190,China;
3. Chinese Academy of Sciences,Beijing 100049,China
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History
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Received |
Revised |
30 Apr 2018 |
05 Jun 2018 |
Issue Date |
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20 May 2022 |
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References
[1] HARRISON A, BOGGS S, CHRISTENSEN F, et al. The nuclear spectroscopic telescope array(NuSTAR)[J]. Astrophysical Journal,2013,770(103):347-356
[2] LEAHY A. Searches for pulsed emission: improved determination of period and amplitude from epoch folding for sinusoidal signals[J]. Astronomy and Astrophysics,1987(180):275-277
[3] BUCCHERI R, BENNETT K, BIGNAMI F, et al. Search for pulsed gamma-ray emission from radio pulsars in the COS-B data[J]. Astronomy and Astrophysiscs,1983(128):245-251
[4] HARTOG R, KUIPER L, HERMSEN W, et al. Detailed high-energy characteristics of AXP 4U 0142+61 multi-year observations with INTEGRAL, RXTE, XMM -Newton and ASCA[J]. Astronomy and Astrophysics,2008(4):1-20