Basic Information on listobs

Task: listobs
Purpose: Makes a summary of a set of observations.
Categories: utility

LISTOBS makes a summary of a set of observations.  Parameters of
interest to the observer are pulled from one or many files, and
printed to a log file.  A time ordered summary of the sources
observed is compiled.  The primary use of this program is to
create a summary of the instrument setup and all observations
made during a track.  Use wild cards or an include file to specify
all files relevent for your observations.
Scans are reported where source name, tsys, were changed.
For more details on the correlator setup, use
uvlist options=spectra vis=...
or
uvindex vis=...

Key: vis
This is the normal keyword for an input visibility dataset. There
is generally no default input name. Some tasks allow multiple input
datasets (with wildcards supported, such as an asterisk). Other tasks
can handle only a single dataset at a time.

Key: log
Output device. (default is standard user output)

Key: options
This gives extra processing options. Several options can be given,
each separated by commas. They may be abbreivated to the minimum
needed to avoid ambiguity.
  'nobase'      Do not list baselines. Useful for big arrays such
                as ATA. By default baselines and uvdistance are
                listed.

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