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Recent work highlights that tens of Galactic double neutron stars are likely to be detectable in the millihertz band of the space-based gravitational-wave observatory, LISA.
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We note that LISA is sensitive to gravitational waves at frequencies below 1 mHz 1\,\mathrm{mHz} , but we focus on ≳ 1 mHz \gtrsim 1\,\mathrm{mHz} since binaries in this band are easier for LISA to detect, and they are more relativistic
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Note, this time to merger includes the aforementioned factor of ten penalty, which takes into account the fact that not all double neutron stars will are likely to include a visible pulsar
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