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        [ASTRO\]UV_TRACKS   station1   station2  [station3  [...]]   [/FRAME
    [size]]  [/HORIZON Elmin] [/HOUR_ANGLE  Hmin  [Hmax]]  [/INTEGRATION  t]
    [/STATIONS ALL|list] [/TABLE [Name]] [/WEIGHT Mode]

    Plot  interferometer UV tracks as observed with the interferometer.  The
    default is for NOEMA, but the command is more general and  can  be  used
    with any array, especially ALMA.

    Station  coordinates  are  searched  for  in the file defined by the AS-
    TRO_STATIONS logical variable. Stations  should  be  referred  to  by  a
    mnemonic  (e.g. E03, W00 ...) given as arguments of UV_TRACKS.  See also
    /STATIONS option.

    Some configuration files for NOEMA and ALMA are distributed with  gildas
    and  can be used as ASTROTIONS files combined with UVTRACKS ALL to avoid
    typing a lot of station names (see HELP UVTRACKS NOEMA or HELP  UVTRACKS

    The  coordinates of the most recently selected SOURCE or PLANET are con-
    sidered. The frequency of the simulated observation is read from the Sic
    FREQUENCY variable (which is also set by LET FREQUENCY command).

    UV_TRACKS  can be used iteratively, to simulate the observations of sev-
    eral configurations. Option /FRAME indicate the start of a new  observa-
    tions:  if  not present, configurations are being stacked on the current
    UV coverage. The user may select another color pen to  distringuish  be-
    tween the various coverages. A sketch of the interferometer described by
    ASTRO_STATIONS is also drawn, and  the  selected  stations/antennas  are


Gildas manager 2019-02-19