“…Van Buchem et al (2011) reported that K120 MFS is of early Cenomanian age, with its highstand extending into the early middle Cenomanian. K130 MFS is of middle Cenomanian age with an associated underlying distinctive sequence boundary (SB) within the early part of the middle Cenomanian (see also van Buchem et al 1996;Schulze et al, 2003Schulze et al, , 2004Schulze et al, , 2005Bauer et al, 2003;Homewood et al, 2008;Saber et al, 2009;Razin et al, 2010;Hajikazemi et al, 2010;Grélaud et al, 2010;Hollis, 2011;Ghanem et al, 2012;Rahimpour-Bonab et al, 2012;Ghanem and Kuss, 2013;Wilmsen and Nagm, 2013;Assadi et al, 2016, for examples of this event across the Arabian Plate). Correlation with the global mid-Cenomanian sea level low (Hancock, 2004;Gale et al, 2008) and 95.5 Ma sequence boundary of Haq (2014) seems likely.…”