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Commit 28461dcd authored by Trent Hare's avatar Trent Hare
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additional updates to the README for current instrument status and reported errors.

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......@@ -44,4 +44,4 @@ For full testing reports and example usage, please see the linked example Jupyte
| Cassini ISS | [link](examples/cassini_isis_cmp.ipynb) | No | sample mean=-12.3; line mean=-0.1 | sample mean=-0.2; line mean=0.9 |
| Dawn Framing Camera | [link](examples/dawn_fc_isis_cmp.ipynb) | sub-pixel; in testing for production | sample mean=-1.9e-03; line mean=1.8e-03 | sample mean=1.9e-03; line mean=-1.8e-03 |
The Difference column (CSM -> ISIS) represents the mean difference in pixels from running usgscsm's *image2ground* from the CSM and then ISIS3's *campt* (ground2image). The Difference column (ISIS -> CSM) is simply the reverse starting with ISIS3 first with *campt* (image2ground) and then usgscsm's *ground2image*.
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The Difference column (CSM -> ISIS) represents the mean difference in pixels from running usgscsm's *image2ground* and then back to the camera using ISIS3's *campt* (ground2image). The Difference column (ISIS -> CSM) is simply the reverse starting with ISIS3 first with *campt* (image2ground) and then usgscsm's *ground2image*.
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