SKAO timing of a handful of binary pulsars can reach unprecedented sensitivity to microhertz gravitational waves from inspiralling massive black hole binaries via resonant perturbations.
Gravitational wave astronomy with the SKA
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VLBI astrometry of nearby MSPs can supply the distance priors needed to localize individual continuous-wave nanohertz GW sources to ~10^{-3} deg².
Review of coincident GW-EM and multi-band GW detections of massive black hole binaries using LISA and SKAO, finding radio counterpart numbers insensitive to jet models.
TransitionListener v2.0 supplies an end-to-end pipeline from scalar potential to gravitational wave spectra with improved handling of transition dynamics and bubble separation.
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TransitionListener v2.0 -- Robust gravitational wave predictions for cosmological phase transitions
TransitionListener v2.0 supplies an end-to-end pipeline from scalar potential to gravitational wave spectra with improved handling of transition dynamics and bubble separation.