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Basic Information on smablsrc


Task: smablsrc
Purpose: Creates a uv dataset of pseudo-point sources.
Categories: uv analysis

SMABLSRC creates a uv dataset of pseudo-point sources, dividing 
the channel data by the continuum vector.

Key: vis
The name of the input uv data sets. Several can be given (wild
cards are supported). No default.

Key: select
The normal uv selection commands. The default is to do every data
points.

Key: line
The normal uv linetype in the form:
  line,nchan,start,width,step
The default is all channels (or all wide channels if there are no
spectral channels). The output will consist of only spectral or
wideband data (but not both).

Key: ref
The normal reference linetype, in the form:
  line,start,width
The default is no reference line.

Key: stokes
If a value is given, smablsrc converts the input into the required
polarizations before writing to the output. Default is to copy
across the polarizations present in the input files.

Key: options
This gives extra processing options. 
   avechunk    do chunk based average.

Key: out
The name of the output uv data set. No default.

User Guide References to smablsrc

[ Basic Info | References | User Guide ]

Generated by smamiriad@cfa.harvard.edu on 09 Jul 2012