Laboratory-derived rate-and-state models depict different evolution of pre-slip within nucleation zones of various sizes (Ampuero & Rubin, 2008; Kaneko & Ampuero, 2011). With technological advances such as high-speed photoelastic techniques, the progressive acceleration from slow stable slip to fast dynamic slip can be accurately monitored in laboratory conditions (e.g., Latour et al., 2013). Despite these advances, the detectability of such nucleation phases on natural faults is still an open question. In addition to the nucleation itself, observations of the precursory phase leading to an earthquake indicate that earthquakes are often preceded by foreshocks that could potentially be triggered by aseismic pre-slip (Bouchon et al., 2011, 2013; Kato et al., 2012). Nonetheless, the role of foreshocks during this precursory phase remains unclear. At present, two end-member conceptual models compete in explaining the occurrence of foreshocks. In the first model, foreshock stress changes contribute to a slow cascade of random failures, leading eventually to the mainshock (Ellsworth & Bulut, 2018; Helmstetter & Sornette, 2003; Marsan & Enescu, 2012). The second model proposes that foreshocks are triggered by aseismic slip corresponding to the nucleation process of the mainshock (Bouchon et al., 2011; Dodge et al., 1996). The continued development of geophysical networks in active tectonic regions provides new opportunities to better capture the genesis of earthquakes. Geodetic observations provide strong evidences of preseismic transient deformations at various timescales (