= Summary of MD.GR1 -- in progress -- =
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(back to [wiki:MediumDeepFields] summary)

Preparation thoughts for the next/uniform MD processing.

All processing (at least per field) really should be done as a unit, no more mix and match.. 

Before it can start
 * V3 -- is it what is wanted, do centers need to be re-shifted? 
 * problem chips/cells/skycells flagged and fixed if possible
 * can edges be dealt with better (do they need to be?)
 * stack types (iq, ref, deep, nightly, convolved) tested and defined (any cuts, minimum inputs, convolved version etc)
 * diffim improvements, photometry tests
 * staticsky/skycal tests


General guideline and stages (stacks/diffs) to do:
 * chip->warp: by default must do
 * stacks: all types now?
  * best IQ/FWHM: what about "poor" edges? best IQ or only make skycell if IQ<X pixels with N inputs?
  * reference stack:
   * all out of season
   * each season/year stack 
  * deep stack:
  * night stack: all during night even if some "marginal"?
 * diffims: which ones need to be done?
  * night WS,SS with with out-of-season refstack or ?
 * staticsky/skycal:


Define uniform label, data_group formats: label and data_group similar ?
 * chip->warp: MD<##>.GR1.<proc start date>
 * stack:
  * reference stack: MD<##>.GR1.<proc start date of chip->warp>.refstack.<proc date> ?
  * deep stack: MD<##>.GR1.<proc date of chip->warp>.deepstack.<proc date>
  * night stack: MD<##>.GR1.<proc date with chip->warp>.nightstack.<obsdate>
 * diffim:
 * staticsky/skycal:


Distribution and cleanup:
 * what goes to distribution this time (who needs what)
 * how long must it stay on disk 
 * what past processing can be cleaned up on disk now