We present the timing results for the binary millisecond pulsar J1640+2224 obtained with the RT-64 radio telescope (TNA-1500, Special Design Bureau, Moscow Power Engineering Institute) at the Kalyazin Observatory (Astrospace Center of the Lebedev Institute of Physics) in 1997–2002. We obtained Keplerian and post-Keplerian parameters of the binary system, which allowed us to estimate an upper limit for the energy density of the stochastic gravitational-wave background radiation at very low frequencies.
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Potapov et al. (2003) studied this question.
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