The pulsar timing residuals induced by gravitational waves from non-evolving single binary sources with general elliptical orbits are *** different orbital eccentricities,the timing residuals present different *** sta...
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The pulsar timing residuals induced by gravitational waves from non-evolving single binary sources with general elliptical orbits are *** different orbital eccentricities,the timing residuals present different *** standard deviations of the timing residuals induced by a fixed gravitational wave source are calculated for different values of the *** also analyze the timing residuals of PSR J0437-4715 induced by one of the best known single gravitational wave sources,the supermassive black hole binary in the blazar OJ287.
PACS:99.10.−x,***,***,*** DOI:10.1088/0256-307X/30/11/119901 One regrettable error appeared in Eq.(21)of our article[***.30(2013)100402].The cor-rect one of the equation is as follows.
PACS:99.10.−x,***,***,*** DOI:10.1088/0256-307X/30/11/119901 One regrettable error appeared in Eq.(21)of our article[***.30(2013)100402].The cor-rect one of the equation is as follows.
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