“…Reported dates and percent discordance for grains younger than 850 Ma are 206 (Ramos, 2004(Ramos, , 2009Bahlburg et al, 2009;Rapela et al, 2016); (2) The Eastern Sierras Pampeanas (725-520 Ma) age group are recycled from Carboniferous to Permian sedimentary sequences found in the Precordillera fold-thrust belt (Fosdick et al, 2015;Capaldi et al, 2017 (Rapela et al, 2007;Schwartz et al, 2008); 3 (Mpodozis and Kay, 1992;Dahlquist et al, 2013) and minor recycled sources from Triassic sedimentary deposits in the Sierras Pampeanas and Neogene deposits throughout the Frontal Cordillera, and Precordillera (Fosdick et al, 2015(Fosdick et al, , 2017; (5) Permian Triassic 280-205 Ma age group includes dominant Choiyoi Igneous Complex and subsequent Triassic plutons exposed in the Frontal Cordillera ( Figure 2B; Mpodozis and Kay, 1992;del Rey et al, 2016). Additional sources of Permian Triassic 280-205 Ma age components include recycled Jurassic to Cretaceous sedimentary deposits in the High Andes and Neogene deposits across the Precordillera (Capaldi et al, 2017;Mackaman-Lofland et al, 2019); (6) Andean Arc 120-0 Ma Cretaceous to Neogene Andean arc volcanic and volcaniclastic rocks of the Principal Cordillera, Frontal Cordillera, Precordillera, and Sierras Pampeanas, and recycled from Neogene basin fill (Kay and Mpodozis, 2002;Jones et al, 2015).…”