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Timing of Binary Pulsars at Kalyazin, Russia

  • Yu. P. Ilyasov (a1), V. V. Oreshko (a1), V. A. Potapov (a1) and A. E. Rodin (a1)

Abstract

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.

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References

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

Timing of Binary Pulsars at Kalyazin, Russia

  • Yu. P. Ilyasov (a1), V. V. Oreshko (a1), V. A. Potapov (a1) and A. E. Rodin (a1)

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