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Hi all,

Just a quick summary of what we decided today:

1) We basically all agree on the main aims of the paper at this point.
They should be:
   i) Present the new FORS calibration scheme as the highly sophisticated,
   integrated, and efficient, automatic, multipurpose calibration method,
   master reduction tool, and secondary standard star catalogue machine
   which we believe it is :)
   ii) Present the first set of new data for Stetson standards (in
   particular the U-band data).
  
2) We were all more or less in agreement about the content of the paper
draft to Sect 3.2.

3) The bits about the TSI, Illum Correction frames, PTPEMs etc need to
be clarified.

Wolfram Action: Provide a section on the large scale filtering
algorithm and provide the filtering scale.

4) Sanity checks should be carried out to see if the iterative procedure
in Sect 3.4 would produce anything else than a corrective F(x,y) = 1.000
frame.

5) The results should be illustrated with Figures showing the TEMs and
example TSIs in all bands.

6) Aim for publication in PASP

7) Wolfram to call meeting next week to discuss the issue of Photometry
and choice of parameters in more detail.

Thats all folks,
:-Pm
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