“…On the other hand, the relatively depleted δ 18 O values (from −7.45 to −5.13‰ VPDB ) suggests formation from relatively high temperature fluids (Allan & Wiggins, ; Spötl & Pitman, ). In this regard, saddle dolomite is considered to precipitate from hot basinal, frequently hydrothermal, fluids (Davies & Smith, ; Mansurbeg et al, ; Morad, Nader, Morad, Al Darmaki, & Hellevang, ), with temperatures above 60°C (Spötl & Pitman, ). Therefore, the most probable scenario is that RD3 and SD1 formed from light carbon and high temperature Mg‐rich fluids expelled from the Zawyat Ahançal Group sediments or the Pliensbachian basinal marls, which are in lateral contact with the Pliensbachian platform carbonates, using faults, fractures and the margin of the Tazoult salt wall as major conduits (Figure ).…”