Notes. The first column corresponds to the identification number present on the global maps in Sect. 3. They are ordered from west to east and from north to south. The second column is the name of the formation, while the last two correspond to the longitude and latitudecoordinates. All the formations are impact craters, except for Vendimia Planitia, Hanami Planum, and Ahuna Mons. ^(a) Vendimia region is a planitia,i.e. a plain of low altitudes interpreted to be an ancient crater basin (Marchi et al. 2016). It includes the Dantu and Kerwan craters. Coordinates are from Stephan et al. (2018); Preusker et al. (2016); Roatsch et al. (2016b). See also Fig. B.1. ^(b) Hanami region is a planum, i.e. a plateau of high altitudes. It includes the Occator crater. Coordinates are derived from Buczkowski et al. (2018). See also Fig. B.1. ^(c) Ahuna Mons is the highest mountain on Ceres and very likely cryovolcanic in origin (Ruesch et al. 2016). ^(d) Oxo is not completely visible on the maps in Sect. 3, due to the Mollweide projection and its location on the meridian of origin. Oxo is seen in Fig. 14 in Sect. 4.7.