“…There is no consensus on the tectonothermal evolution of the HCM and several contradicting models have been proposed. Most authors (Bełka, ; Marynowski, , ; Marynowski, Salamon, & Narkiewicz, ; Naglik, Toboła, Natkaniec‐Nowak, Luptáková, & Milovská, ; Narkiewicz, ; Narkiewicz, Resak, Littke, & Marynowski, ; Smolarek, Marynowski, Spunda, & Trela, ) argue for an elevated Variscan (late Carboniferous to early Permian) heat flow, which significantly exceeded the current low values (Szewczyk & Gientka, ). However, Poprawa, Żywiecki, and Grotek () proposed that thermal maturity of organic matter in the Devonian to Jurassic sedimentary successions was achieved during Late Jurassic or Late Cretaceous burial that was characterized by constant heat flow equal to the recent one (Szewczyk & Gientka, ).…”