White dwarf–Intermediate-Mass Black Hole Inspirals (WD-IMRI) are promising mul-timessenger (MS) sources, producing gravitational waves and electromagnetic radiation when they undergo tidal stripping. We search for systems with the necessary conditions to trigger these multimessenger signals in WD-IMRIs and their formation mechanisms in around 2,000 globular clusters from the MOCCA Survey 1. We also analyze their multimessenger detectabil-ity; our results suggest that these systems are detectable by the upcoming GW observatories such as LISA, TianQin, and Taiji, and by X-ray telescopes such as the Einstein Probe.
