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1812<br />
1813<br />
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1818<br />
material has been observed throughout the system, and there is some evidence that this<br />
contamination might also be a relatively recent process.<br />
Acknowledgements: We gratefully acknowledge the long years <strong>of</strong> work by the entire Cassini team that allowed these<br />
data <strong>of</strong> the Saturnian satellites to be obtained. We should also like to thank NASA, ESA, ASI, DLR, CNES and JPL for<br />
providing support for the international Cassini team. We thank K. Stephan, R. Wagner and M. Langhans for data<br />
processing. The discussions <strong>of</strong> reviewers C. Chapman and D. Domingue are highly appreciated. Part <strong>of</strong> this work was<br />
performed at the DLR Institute <strong>of</strong> <strong>Planetary</strong> Research, with support provided by the Helmholz Alliance ’<strong>Planetary</strong><br />
Evolution and Life’ and the Jet Propulsion Laboratory under contract to the National Aeronautics and Space<br />
1819 Administration.<br />
We dedicate this work to Steve Ostro, who provided outstanding scientific contributions to the exploration <strong>of</strong> the<br />
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1821<br />
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Saturnian System.<br />
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