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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 

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