Over the past 20+ years, broadband seismometers and continuous global positioning system (GPS) networks have combined to illuminate a continuum of fault slip behaviors. These observations show that tectonic faults store and release elastic-strain energy through a spectrum of slip regimes ranging from slow, aseismic slip to fast, dynamic earthquake ruptures (e.g., Behr & Burgmann, 2020;Beroza & Ide, 2011;Peng & Gomberg 2010). Slow earthquakes encompass a range of slip modes that include aseismic creep, very-low frequency earthquakes (VLFE), low-frequency earthquakes (LFE), non-volcanic tremor (NVT), and episodic tremor and slip (ETS) (Obara, 2002;Rogers & Dragert, 2003;Shelly et al., 2007). Since the discovery of slow earthquakes, a fundamental goal in earthquake seismology has been to elucidate the connections, and the possibility of fundamental differences, between slow and regular earthquakes (Obara & Kato, 2016). If the underlying physics associated with slow earthquakes is similar to that of ordinary earthquakes, then we can use observations of slow earthquakes to