Pipeline & DS20

[Michael Sallman <msallman@pro-ns.net>]

Michael and all,

Over the weekend I tried to run some of DS 20 through Michael's
pipeline.
I used disks 1 & 2 (the light box bias/dark/flat for V & I) to generate
the master_dark_* and master_flat_*, and disks 9 & 10 for the objects. I
was able to run through the entire pipeline.
The results :

1 calibrated set of images (Mhra2246777.cal)
3 collated sets of images (Mhra2246777.clt, Mhra2246791.clt,
Mhra2246804.clt)
3 .ast files for 56 I images
56 .ast files for 56 V images.

The values from Mhra2246777.coeff :
V=V,(V-I)  N    160  a  -8.667  0.010  b  -0.052  0.014   RMS  0.065
I=I,(I-V)  N    160  a  -8.639  0.010  b  -0.067  0.013   RMS  0.130

I am currently reading TN76 and re-reading the pipeline.html documents.
Looks like my first step is to try adjusting the RA/Dec of the I files?
Any other suggestions would be appreciated.

On the bright side, I now have 1039 calibrated stars to work with. Now
all I have to do is get a database set up and I'm off to the races.

Thanks,
Mike