“…In the past decades, several studies focused on fault‐fluid interactions through the structural, geochemical, and geochronological characterization of syn‐tectonic mineralization in specific fault zones pertaining to fold‐and‐thrust belts (Agosta & Kirschner, 2003; Agosta, 2008; Beaudoin et al., 2011; Dennis et al., 2019; Dewever et al., 2013; Huntington & Lechler, 2015; Lacombe & Beaudoin, 2024 for review; Lacroix et al., 2011; Lucca et al., 2019; Marchesini et al., 2022 Smeraglia et al., 2016, 2018). However, a few studies attempted to characterize the spatio‐temporal fluid paleo‐circulation along transects tens to hundreds of kilometers long (Callot et al., 2010; Crognier et al., 2018; Fitz‐Diaz et al., 2011; Kirschner & Kennedy, 2001; Knoop et al., 2002; Vandeginste et al., 2012), and rarely at scales covering entire fold‐and‐thrust belts (Beaudoin et al., 2014, 2022 for review; Cruset et al., 2023; Ghisetti et al., 2001; Smeraglia et al., 2022; Travé et al., 2007).…”