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Timing of Binary Pulsars at Kalyazin, Russia

Published online by Cambridge University Press:  19 July 2016

Yu. P. Ilyasov ,
V. V. Oreshko ,
V. A. Potapov  and
A. E. Rodin
Yu. P. Ilyasov
Affiliation:
Pushchino Radio Astronomy Observatory, P. N. Lebedev Physical Institute, 142290, Pushchino, Russia
V. V. Oreshko
Affiliation:
Pushchino Radio Astronomy Observatory, P. N. Lebedev Physical Institute, 142290, Pushchino, Russia
V. A. Potapov
Affiliation:
Pushchino Radio Astronomy Observatory, P. N. Lebedev Physical Institute, 142290, Pushchino, Russia
A. E. Rodin
Affiliation:
Pushchino Radio Astronomy Observatory, P. N. Lebedev Physical Institute, 142290, Pushchino, Russia

Abstract

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Regular high-precision timing of the binary pulsars J0613−0200, J1012+5307, J1022+1001, J1640+2224, J1643−1224, J1713+0747, J2145−0750 and the pulsar B1937+21 has been conducted at the Kalyazin (Russia) radio telescope RT-64 at 0.6 GHz over more than 6 years. Several of the pulsars monitored have been found to be good probes for gravitational wave background (GWB) tests, while others, having a shorter orbital period, can be used for establishing a dynamical binary pulsar timescale. Upper limits for the GWB energy density were estimated.

Type
Part 10: Radio Pulsar Timing
Information
Symposium - International Astronomical Union , Volume 218: Young Neutrons Stars and their Environments , 2004 , pp. 433 - 434
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Doroshenko, O. V., & Kopeikin, S. M. 1990, Sov. Astr., 34, 496.Google Scholar
Ilyasov, Yu. P., Oreshko, V. V., & Doroshenko, O. V. 2000, in Proc. LPI. 229, p. 95.Google Scholar
Ilyasov, Yu. P., Poperechenko, B., & Oreshko, V. V. 2000, in Proc. LPI. 229, p. 44.Google Scholar
Kopeikin, S. M., 1997, Phys. Rev. D, 56, 4455.Google Scholar
Matsakis, D. N., Taylor, J. H., & Eubanks, T. M. 1997, A&A, 326, 924.Google Scholar
Taylor, J. H., & Weisberg, J. M. 1989, ApJ, 345, 434.CrossRefGoogle Scholar