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Last Night
I collected 24 x 180 = 4320 square degrees of the sky last night with
TOM1. This is 1/10 of the whole sky. When I run TOM2 and TOM3 this will
be 3/10 of this sky on a winter night and half that on a summer night. But
it is really twice that for the sky I can see.
This is not yet "good" data. But it is still possible to use it to pick
out variable star candidates as a number of you can attest.
The black flocked paper came in. It really looks "black" when you look at
it head on. When you look at it at a shallow grazing angle (where it
really has to work) it is not as black. Sigh! Possibly we will need the
black paint and walnut shells. (This is not yet a call for you to save
your Christmas stocking walnut shells for me.)
While I was writing this, UPS came and I have the stiffeners. I just
installed them in the V camera and it looks like they do the job. At least
the focus for the V camera is now very smooth. They came in anodized a
pretty blue. So we add some color to the Mark IV. As soon as I get clear
sky I will test the focus with the new stiffeners.
Meanwhile I have a plan to use xvista to remove the natural sky gradient in
the proper order for computation. Michael's tools are very nice and easy
to use. His man pages give lots of useful examples. This is something I
notice that unix avoids.
So progress is progressing. I have great hope to start a real survey in
March.
Tom Droege