  Pulsars (PSRs) orbiting intermediate or supermassive black holes at the
centre of galaxies and globular clusters are known as Extreme Mass Ratio
Binaries (EMRBs) and have been identified as precision probes of strong-field
GR. For appropriate orbital parameters, some of these systems may also emit
gravitational radiation in a `burst-like' pattern. The observation of this
burst radiation in conjunction with the electromagnetic radio timing signal
would allow for multimessenger astronomy in strong-field gravitational regimes.
In this work we investigate gravitational radiation from these PSR-EMRBs,
calculating the waveforms and SNRs and explore the influence of this GW on the
pulsar radio signal. We find that for typical PSR-EMRBs, gravitational burst
radiation should be detectable from both the Galactic centre and the centre of
stellar clusters, and that this radiation will not meaningfully affect the
pulsar timing signal, allowing PSR-EMRB to remain `clean' test-beds of
strong-field GR.
