A mathematical method for the de-dispersion of the pulsar profile

Author:

Yuan JianPing,Wang Na,Wu XinJi,Esamdin Ali

Publisher

Springer Science and Business Media LLC

Subject

General Physics and Astronomy

Reference6 articles.

1. Large M I, Vanghan A E. A search of the galactic plane for high dispersion pulsars. MNRAS, 1971, 151: 277–287

2. Wu X J, Liu X F. An arithmetic method for mean pulse profile de-disperse of pulsars. In: Kramer M, Wex N, Wielebinski N. eds. Pulsar Astronomy—2000 and Beyond, ASP Conference Series, Vol. 202. San Francisco: ASP, 2000. 285–286

3. Wang N, Manchester R N, Zhang J, et al. Pulsar timing at Urumqi Astronomical Observatory: Observing system and results. MNRAS, 2001, 328: 855–866

4. Krishnamohan S, Downs G S. Intensity dependence of the pulse profile and polarization of the VELA pulsar. Astrophys J, 1983, 265: 372–388

5. Wu X, Xu W, Rankin J M. On the separation of the components in the mean pulse profile of PSR 1451-68 and their spectral behavior. In: Magnetospheric Structure and Emission Mechanics of Radio Pulsars, Proceedings of IAU Colloq. 128. Poland: Pedagogical University Press, 1992. 172–175

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1. Some recent progress in study of gravity and cosmology;Chinese Science Bulletin;2012-12

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