Automatic online Quality determination

  After your observations have been done, the current observer will run a ``quality'' script that is used to derive some quality parameters of the observation. There are a few parameters to this quality program that have to be ``guessed'' by the observer. Although they generally do have your observing script available, it can be a great help if you supply them with the correct parameters. These are a list of the kind (phase, amplitude, passband) calibrators you are using for your run.

An example:

    setup name=quality p= s= 

    s=      visbility dataset(s) that are the source
    p=      same, for passband calibrators
    g=      same, for phase calibrator
    a=      same, for amplitude calibrator