<?xml version='1.0' encoding='utf-8'?>
<oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
  <dc:contributor>E. Kersten</dc:contributor>
  <dc:contributor>K.-D. Matz</dc:contributor>
  <dc:contributor>Michael T. Bland</dc:contributor>
  <dc:contributor>Tammy L. Becker</dc:contributor>
  <dc:contributor>Gerald Wesley Patterson</dc:contributor>
  <dc:contributor>C. Porco</dc:contributor>
  <dc:creator>Thomas Roatsch</dc:creator>
  <dc:date>2018</dc:date>
  <dc:description>&lt;p&gt;&lt;span&gt;The Imaging Science Subsystem (ISS) on-board Cassini took a few high-resolution images of the icy Saturnian satellites&amp;nbsp;Mimas&amp;nbsp;and&amp;nbsp;Enceladus&amp;nbsp;over the last seven years of the&amp;nbsp;Cassini mission&amp;nbsp;during non-targeted flybys. We used the new Mimas images to improve the existing semi-controlled mosaic of Mimas. A new controlled Enceladus mosaic was published recently (Bland et&amp;nbsp;al., 2015; Bland et&amp;nbsp;al. in prep.). Both new mosaics are the baseline for improved atlases of Mimas in three tiles with a map scale of 1:1,000,000 and Enceladus in 15 tiles with a map scale of 1:400,000. The&amp;nbsp;&lt;/span&gt;nomenclature&lt;span&gt;&amp;nbsp;for both satellites was proposed by the Cassini-ISS team and approved by the IAU.&lt;/span&gt;&lt;/p&gt;</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.1016/j.pss.2018.05.021</dc:identifier>
  <dc:language>en</dc:language>
  <dc:publisher>Elsevier</dc:publisher>
  <dc:title>Final Mimas and Enceladus atlases derived from Cassini-ISS images</dc:title>
  <dc:type>article</dc:type>
</oai_dc:dc>