In time, just before the Cassini Iapetus flyby I did a preliminary DEM of a small area of Iapetus' surface:
Click to view attachment
The area it covers:
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I created the DEM from a stereo pair using software I have been developing (see this thread for more information).
The DEM is based on images with somewhat inaccurate viewing geometry - the pointing information in the PDS files really isn't accurate enough for my purposes. This is difficult to correct, in part because of Iapetus' somewhat irregular shape. I probably need to establish a global control point network to determine the exact pointing but there's a catch-22: To make it easier I really need accurate pointing information for at least one image but this is difficult to determine without a control point network...
In the DEM the difference between black (lowest) and white (highest) is 33 km. This is highly inaccurate because of the viewing geometry inaccuracies mentioned above. An obvious 'proof': Distances from Iapetus' center range from 785 to 818 km according to my stereo software. This cannot be correct, the best-fit triaxial ellipsoid has been determined to be 747.1 x 749.0 x 712.6 km. However, relative elevations over fairly small areas should be reasonably accurate so things like crater depths can be estimated. For example the depth of the crater centered at ~(380,220) is ~3.5 km.
A lot of additional imaging coverage is available so I should be able to make a bigger DEM once I have determined accurate pointing for the images I will be using.