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Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 1(477), p. 964-976

DOI: 10.1093/mnras/sty689

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Single sources in the low-frequency gravitational wave sky: properties and time to detection by pulsar timing arrays

This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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