Wayne Landsman discussed the FUV MAMA dark. The dark rate is 10 times the diffuse UV background. Sally said that a dark splotch in which many of the counts are localized happens sometimes but not at other times, and the splotch is correlated with temperature. Don said there are other sources of variance also, not just temperature. The FUV MAMA dark is being applied to the HDF parallel.
Some asymmetry is left in the splotch.
We now have 100 dark frames. The results are the same as those from Eliot's standalone code to a very small fraction of a pixel. An emission line object has been found. Nick Collins has reprocessed the HDF parallels to use the whole exposed image data, not just the intersection of all the dithers. He is having problems getting rid of the NUV window glow, which is not symmetric.