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Measurement and correction of variations in interstellar dispersion in high-precision pulsar timing

Monthly Notices of the Royal Astronomical Society, no. 3 (2013): 2161-2174

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Signals from radio pulsars show a wavelength-dependent delay due to dispersion in the interstellar plasma. At a typical observing wavelength, this delay can vary by tens of microseconds on 5-yr time-scales, far in excess of signals of interest to pulsar timing arrays, such as that induced by a gravitational wave background. Measurement of...更多

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