“…Tapers higher than 4° are common in the fronts of accretionary prisms, FTB or gravity systems which are detached in overpressured shale rocks (Dahlen & Suppe, 1984;Morley et al, 2011;Suppe, 2007;Tuitt et al, 2012;Yang et al, 2016;Yue & Suppe, 2014). High taper values, like those of the Chartreuse and Vercors massifs, are in the range of tectonic wedges like the Barbados accretionary prism (8°; Casey- Moore et al, 1988), the Sabah prism (10°; Hall & Wilson, 2000), the Makran accretionary prism (10°; Ellouz- Zimmermann et al, 2007), the Hikurangi accretionary prism in New-Zealand (10°; Morley et al, 2011), or FTB like the Papua-New Guinea thrust system (12°; Hill, 1991), the Peruvian Sub-Andean thrust system (10°; Baby et al, 2018), or else the cordilleran system in NE Mexico (12°, Deville et al, 2020). Such high taper tectonic wedges are associated with high pressure conditions in overpressured shale at the decollement level close to natural hydraulic fracturing conditions as shown by pressure measurements coupled with numerical modeling in the Barbados accretionary prism (Deville et al, 2010) or the Papua-New Guinea FTB DEVILLE 10.1029/2020TC006591 (Callot et al, 2017).…”