SIMULATE

          IMAGER\SIMULATE [?|Setup|Coverage|Model|Noise|Image|*]
      [/MODEL ModelFile  [Declination]] [/ARRAY Tele]
      [/CONFIGS List of Config] [/HOUR Hours per Config]
      [/NOISE Noise [BandWidth]

        Compute a UV coverage for the specified List of Configuration of the in-
    dicated  telescope  Array,  observing +/- Hours per configuration around the
    transit. Then use the resulting UV table to simulate the observation of  the
    sky brightness given in ModelFile.

        If  the  field  of view of the ModelFile exceeds the primary beam of the
    array, an appropriate Mosaic coverage is computed.

      Thermal noise can be added to the simulated visibilities.

      Actions are (in appropriate sequence order)
      SETUP     Setup the input parameters according to the specified options.
      COVERAGE  Compute Mosaic Pattern and UV coverage
      MODEL     Compute the noise-free simulated UV data
      NOISE     Add noise to the simulated UV data
      IMAGE     Perform the imaging using the noisy simulated UV data
      FIDELITY  Compute Image Fidelity
      In addition, the following arguments are recognized
      ?         List the input parameters
      *         Perform all actions in sequence.