Fourteen planetary-mass companions orbiting pulsars or white dwarfs emit continuous gravitational waves strong enough for detection at S/N ≳5 by future detectors like DECIGO and BBO within four years of observation.
(2018); [33] Neustroev & Mäntynen (2023); [34] Kupfer et al
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Detectability of continuous gravitational waves from planetary-mass companions orbiting compact stars
Fourteen planetary-mass companions orbiting pulsars or white dwarfs emit continuous gravitational waves strong enough for detection at S/N ≳5 by future detectors like DECIGO and BBO within four years of observation.