“…One of the major problems encountered by all investigators was the poor age control of Upper Cretaceous stratigraphic sequences in the Western Desert as a result of a poor fossil record. Exceptions are the outcrops of the Farafra Oasis, which are rich in microfossils (Hottinger, 1960;Said & Kerdany, 1961;Youssef & Abdel Aziz, 1971;Samir, 1994Samir, , 1995Abdel-Kireem & Samir, 1995;Tantawy, 1998), and the Cenomanian deposits of the Bahariya Formation to the north (Slaughter & Thurmond, 1974;Dominik, 1985;Allam, 1986;Werner, 1989;Smith et al, 2001). Consequently, age control in most studies of the Dakhla Formation was limited to assigning an undifferentiated Maastrichtian age, and correlation of sequences was frequently based on the lithology of formations (e.g., upper Campanian Duwi Formation, Maastrichtian Dakhla Formation, Paleocene Tarawan Formation).…”