“…The development of the Cantabrian Orocline requires the existence of a roughly linear orogenic belt during the early Variscan closure of the Rheic Ocean (with a roughly N-S orientation in present-day coordinates), which was subsequently bent in plan view into an orocline during the late stages of Pangea's amalgamation. Such an interpretation is grounded in extensive paleomagnetic studies (e.g., Hirt et al, 1992;Parés et al, 1994;Stewart, 1995;van der Voo et al, 1997;Weil, 2006;Weil et al, 2000Weil et al, , 2001Weil et al, , 2010b, as well as through important contributions from structural (e.g., Gutiérrez-Alonso, 1992;Kollmeier et al, 2000;Merino-Tomé et al, 2009;Pastor-Galán et al, 2011, 2014Shaw et al, 2015) and geochronological studies (e.g., Tohver et al, 2008;Gutiérrez-Alonso et al, 2015). Weil et al (2013) provided a comprehensive review of the kinematic constraints, which were updated by Pastor-Galán et al (2017a) and by Weil et al (2019).…”