Fig. 9
O−C residuals relative to the IMCCE NOE-6-2015-MAIN-Coorb2 ephemeris plotted as line residual versus sample residual. Units are NAC pixels. Enceladus, Hyperion, and Helene are not shown, due to the small number of observations for these satellites, but are included in Tables 2 and 3. One outlier for Mimas (0.2, − 5.6), one for Dione (− 1.0, 5.3), and one for Iapetus (− 5.1, 3.4) are not shown.
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