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Discovery and Timing of Pulsars in the Globular Cluster M13 with FAST

  • Authors: Lin Wang, Bo Peng, B. W. Stappers, Kuo Liu, M. J. Keith, A. G. Lyne, Jiguang Lu, Ye-Zhao Yu, Feifei Kou, Jun Yan, Peng Jiang, Chengjin Jin, Di Li, Qi Li, Lei Qian, Qiming Wang, Youling Yue, Haiyan Zhang, Shuxin Zhang, and Yan Zhu

2020 The Astrophysical Journal 892 43.

  • Provider: AAS Journals

Caption: Figure 9.

S/N variations of the six pulsars in M13. The x-axis is observation ID; long observations are marked with several observation IDs so that the data in each observation ID have similar integration times. The y-axis is S/N divided by ﹩\sqrt{t}﹩. t is the integration time of data in each observation ID.

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