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  1. Integrate measurements from photo-diodes into sky brightness model

  2. Plot of zero-point as a function of time

  3. Automate updating sql database of optical and IR data
  4. Figure out the best way to set the absolute zero-point of the camera
  5. Easy "cloudy" metric?

Stretch Goals

  1. Run uber-cal on the stellar photometry so we can plot transparency as a function of time.

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