“…1A), formed due to the late Paleozoic-early Mesozoic accretion of the Kunlun, Karakul-Mazar, central Pamir, and southern Pamir terranes (Fig. 1B; Burtman and Molnar, 1993;Burtman, 2010;Robinson et al, 2004Robinson et al, , 2012Robinson, 2015;Angiolini et al, 2013;Villarreal et al, 2020;Chen et al, 2021;Li et al, 2022;Rembe et al, 2022) and the late Mesozoic-Cenozoic intracontinental deformation caused by northward subduction of the Neo-Tethys oceanic slab and subsequent collision of the Indian and Asian plates (Burtman and Molnar, 1993;Sobel and Dumitru, 1997;Robinson et al, 2004;Cowgill, 2010;Bershaw et al, 2012;Sobel et al, 2011Sobel et al, , 2013Cao et al, 2013a;Robinson, 2015;Rutte et al, 2017aRutte et al, , 2017bChapman et al, 2018;Worthington et al, 2020;Cai et al, 2021;Li et al, 2022;Villarreal et al, 2023). In this convergent setting, igneous and medium-to high-grade (575-830 °C/6-22 kbar) metamorphic rocks were initially exhumed in the early Miocene in the Pamir interior in a series of gneiss domes that formed by detachment faulting associated with ∼N-S extension (Fig.…”