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126 R. Chemello and S. Silenzi

                                                                                 2.2

                                                                                 2.0

                                                                     d18O (PDB)  1.8

                                                                                 1.6

                                                                                 1.4

                                                                                 1.2 4C dating

                                                                                 1.0            1600  1700       1800      1900  2000
                                                                                   1500

                                                                                                      Calculated years AD

                                                                                                            (a)

Downloaded by [Weizmann Institute of Science] at 03:22 26 June 2013  d18O (PDB) 1.7
                                                                                1.4
                                                                                1.1             1600  1700       1800      1900  2000
                                                                                0.8
                                                                                0.5
                                                                                0.2
                                                                               –0.1
                                                                               –0.4
                                                                               –0.7

                                                                                  1500

                                                                                                      Calculated kyr BP
                                                                                                              (b)

                                                                     Figure 3. The δ118O (‰ PDB) composition of two different transects of the Sicilian Vermetid colonies (a) (modifed from
                                                                     Silenzi et al. [6]) compared with the mean δ18O (‰ VPDB) recorded from the Israeli Mediterranean coast (b) (modified
                                                                     from Sisma-Ventura et al. [7]). The black triangle in (a) represents the calibrated 14C date on which the chronological
                                                                     models of all the three records are based. The dashed lines in the Sicilian records indicate the δ18O value of each section

                                                                     for actual living Vermetids.

                                                                     Acknowledgements

                                                                     This article has been inspired by INTERMED, one of the CIRCLE Med projects funded by the French Ministry of
                                                                     Ecology, Energy, Sustainable Development and Territorial Planning, the Regional Ministry of Innovation and Industry
                                                                     of the Galician Government, the Ministry of Environment Protection of Israel, the Italian Ministry for Environment,
                                                                     Land and Sea, and the Foundation for Science and Technology of Portugal, in the framework of Circle ERA Net project
                                                                     (which is funded by the European Commission 6th Framework Programme). We thank Gianluca Sarà (University of
                                                                     Palermo) for the invitation to the Intermed Workshop, and the following colleagues for their help and useful comments
                                                                     on the manuscript: Marco Milazzo, Mariagrazia Graziano and Silvano Riggio (University of Palermo), Saverio Devoti
                                                                     (ISPRA, Roma), Paolo Montagna (Lamont-Doherty Earth Observatory, Columbia University). We are very grateful to
                                                                     Martina Genovese (Studio Associato Gaia, Genova) and Helen Main (Palermo) for their help during the preparation of
                                                                     the manuscript.

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