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Software Progress
Slowly the software in my head is getting into a file and is being debugged.
I now have the software working that reduces each image to an individual
.cal file. For each .cal file I am looking at the refcat.dat stars that it
contains. I am using DS-24 Set #3 as a test file.
When I compare the .cal magnitude with the refcat.dat magnitude, if find
that the RMS value (sigma) is rather large and rather uniform for the 49
images of DS-24.
Values for V are typically 0.15 mag ranging from 0.14 to 0.16 for the 49
images. Values for I are typically 0.25 mag ranging from 0.24 to 0.27. I
think this tells us what we already knew. We need a better reference
catalog. Since DS-24 moves around in RA-Dec space, the refcat.dat stars
vary from image to image. Typically there are 700 to 900 stars in
refcat.dat for DS-24 #3.
I think DS-23 #3 is the cleanest set with respect to clouds. At least the
cloud removal stage did not reject any images. I did have the limits set
rather high. I will run it again with a tighter cloud rejection limit.
There are enough refcat stars available that I can sort out the ones with
the smallest error. There must be an optimum point between many stars with
large error and too few stars to get a good fit. I also want to go back
and try to bootstrap the refcat again. There are now lots of fun things to
do.
Tom Droege