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Pulsar timing with the DFB at Nanshan

Published online by Cambridge University Press:  20 March 2013

J. P. Yuan ,
N. Wang ,
Z. Y. Liu  and
J. B. Wang
J. P. Yuan
Affiliation:
Xinjiang Astronomical Observatory, CAS, 150 Science 1-Street, Urumqi, Xinjiang, China, 830011 email: yuanjp@xao.ac.cn
N. Wang
Affiliation:
Xinjiang Astronomical Observatory, CAS, 150 Science 1-Street, Urumqi, Xinjiang, China, 830011 email: yuanjp@xao.ac.cn
Z. Y. Liu
Affiliation:
Xinjiang Astronomical Observatory, CAS, 150 Science 1-Street, Urumqi, Xinjiang, China, 830011 email: yuanjp@xao.ac.cn
J. B. Wang
Affiliation:
Xinjiang Astronomical Observatory, CAS, 150 Science 1-Street, Urumqi, Xinjiang, China, 830011 email: yuanjp@xao.ac.cn
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Abstract

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Pulsar timing observations are being carried out with the Nanshan 25-metre radio telescope since 2000. We observe about 300 pulsars, including nine millisecond pulsars, at 1.5 GHz with a cryogenic receiver and digital filterbank. Frequent observations at Nanshan revealed 50 glitches. We detect nine more glitches in the past two years. Timing solutions obtained with the Nanshan telescope for eight radio loud Gamma ray pulsars are presented.

Keywords

stars: pulsars: generaltiming
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S291: Neutron Stars and Pulsars: Challenges and Opportunities after 80 years , August 2012 , pp. 574 - 576
Copyright
Copyright © International Astronomical Union 2013

References

Abdo, A. A., Ackermann, M., Ajello, M.et al., 2010 ApJS, 187, 460CrossRefGoogle Scholar
Espinoza, C. M., Lyne, A. G., Stappers, B. W., & Kramer, M., 2011, MNRAS, 414, 1679CrossRefGoogle Scholar
Hobbs, G. B., Edwards, R. T., & Manchester, R. N. 2006, MNRAS, 369, 655CrossRefGoogle Scholar
Hotan, A. W., van Straten, W., & Manchester, R. N. 2004, PASA, 21, 302CrossRefGoogle Scholar
Smith, D. A., Guillemot, L., Camilo, F.et al., 2008, A&A, 492, 923Google Scholar
Wang, N., Manchester, R. N., Zhang, J., et al. 2001, MNRAS, 328, 855CrossRefGoogle Scholar
Wang, J. B., Wang, N., Tong, H., & Yuan, J. P., 2012, ApSS, 340, 307Google Scholar
Yuan, J. P., Wang, N., Manchester, R. N., & Liu, Z. Y. 2010a, MNRAS, 404, 289Google Scholar
Yuan, J. P., Manchester, R. N., Wang, N., et al. 2010b, ApJL, 719, L111CrossRefGoogle Scholar
Zou, W. Z., Wang, N., Wang, H. X., et al. 2004, MNRAS, 354, 811CrossRefGoogle Scholar
Zou, W. Z., Wang, N., Manchester, R. N., et al. 2008, MNRAS, 384, 1063CrossRefGoogle Scholar