“…These Cretaceous anoxic events are well documented since the Valanginian (e.g., Lini et al, 1992;Aguirre-Urreta et al, 2008) through the Santonian (Wagreich, 2012). Such an event is widely recognized as OAE1a which characterizes lower Aptian sediments (e.g., Schlanger and Jenkyns, 1976;Arthur, 1979;Arthur et al, 1990;Koutsoukos et al, 1991a;Koutsoukos et al, 1991b;Kuhnt et al, 1998;Masse and Machhour, 1998;Menegatti et al, 1998;Mutterlose and Böckel, 1998;Scarparo Cunha and Koutsoukos, 1998;Larson and Erba, 1999;Maurrasse and Ponton, 2005;Coccioni et al, 2006;Abu-Zied, 2007;Barragán and Maurrasse, 2008;Michalík et al, 2008;Yilmaz, 2008;Moreno-Bedmar et al, 2009;Moreno-Bedmar, 2010;Föllmi, 2012;Husinec et al, 2012;Léonide et al, 2012;Roban and Melinte-Dobrinescu, 2012;Elkhazri et al, 2013;Gaona-Narvaez et al, 2013;Socorro and Maurrasse, 2019;Hu et al, 2020;Socorro and Maurrasse, 2020;Herdocia and Maurrasse, 2022;Socorro and Maurrasse, 2022). These studies (herein above) generally agree that different marine physiographic conditions may respond with varieties of facies during OAEs exclusive of black shales and with remarkable differences in degrees of oxygen depletion which may not show OM-rich sediments.…”