“…Further studies confirmed the global distribution of the OAE 1d subevents; for instance, studies from the northwestern Tethys (in the Vocontian Basin, SE France, Bornemann et al, ; Bréhéret, ; Giorgioni et al, ; and in the Pialli Italian Apennines, Coccioni, ), the southern Tethys (in Tunisia, Ben Fadhel, Layeb, Hedfi, & Ben Youssef, ; Talbi, Lakhdar, Smati, Spiller, & Levey, ), the northwestern Atlantic (in Blake Nose Plateau, Watkins, Cooper, & Wilson, ; Wilson & Norris, ), the United States (Scott, Formolo, Rush, Owens, & Oboh‐Ikuenobe, ), and southwestern Venezuela (Rodríguez‐Cuicas, Montero‐Serrano, & Garbán, ). Generally, the OAE 1d is characterized by: (a) a low to moderate positive carbon excursion (0.5–2‰; Bornemann et al, ; Watkins et al, ; Wilson & Norris, ) and TOC contents (1–2 wt%; Bornemann et al, ; Bréhéret, , ; Rodríguez‐Cuicas et al, ); and (b) being a product of stratification collapse in the water column especially in the western tropical Atlantic (Wilson & Norris, ). However, recent studies indicated that OAE 1d was formed due to enhanced orbital forcing mechanisms that led to the development of unstable circulation patterns, which favored expanded deep‐water anoxia (Bornemann et al, ; Giorgioni et al, ).…”