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We acknowledge the individuals at CICLOPS and across the Imaging Team who helped in planning and designing the Phoebe and lapetus sequences and in keeping the imaging operations running smoothly. This paper is dedicated to the memory of Damon Simonelli, who developed much of the pre-Cassini understanding of Phoebe's surface. This work has been funded by NASA/Jet Propulsion Laboratory, the UK Particle Physics and Astronomy Research Council, the German Aerospace Center (DLR), and Université Paris VII Denis Diderot, Commissariat à l'Energie Atomique, Astrophysique Interactions Multiechelles, France.
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