Disk 18 fwhm Plots by CCD column

V Filter Column fwhm plots for several nights

As you can see in the V plots the slope changes quite a bit. disks B-E are quite similar, G is much flatter and the slope decreases over HIJ

What changed between E(F??) and G disks?

Tom writes on README on 18J
"I changed a camera mid way in the run, so you will not be able to use one flat for the whole run."

So that might explain things a bit. Presumably it was the V camera.


I Filter Column fwhm plots for several nights

The I fwhm column plots have two similar forms B-E and G-J.

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