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The data reduction categories covered in this document are those for
continuum data, continuum polarimetry and spectral-line
data. Individual steps in each data reduction sequence are illustrated
using Glish scripts. The reduction sequences given in this document
use the following AIPS++ tools:
- vlafiller
- is used to load VLA archive
uv data into an AIPS++ format called a Measurement Set (MS). The
MS is stored on disk as a directory with a ``table'' name specified
by the user, e.g. 3C273.ms.
- ms
- is used to access uv-data in a Measurement Set,
and to list and summarize visibility data.
- flagger
- is used to select and flag
uv-data in a Measurement Set.
- msplot
- is used for plotting and interactively
editing visibility data. It is also useful to investigate and
edit the data between calibration cycles.
- calibrater
- is used to solve for
uv-plane calibration effects, apply calibration corrections to the
observed data, and plot calibration solutions.
- imager
- is used to image (e.g. Fourier
transform, deconvolve, restore) the data in the Measurement Set.
- image
- is used for image
analysis, e.g. fitting 1-D profiles or 2-D models to images,
creating moment maps, regridding images.
- viewer
- is used to display images and
create publication quality postscript renderings of them. In
addition, image tool statistics are available from within the
viewer. The viewer is also used to create CLEAN
deconvolution regions or masks.
Next: What happens if something goes wrong?
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2004-08-28