| Version 1.9 Build 1556
|
|
Next: Appendix B: Creating your own .aipsrc file
Up: Getting Started in AIPS++
Previous: Frequently Asked Questions
Subsections
To simplify use of AIPS++, the available functionality is
split into a hierachy of packages and modules. One can choose to use
just those packages and modules which are of direct interest.
Each module holds a number of toolsand global functions.
The top layer of the AIPS++ software system contains
packages.
Each package contains specific modules. Some examples of packages are:
- synthesis
- : for processing
aperture synthesis data with modules for calibrating, editing,
visibility plotting, imaging, and deconvolving.
- general
- : contains modules of general utility
such as units and measures, coordinate conversions, image analysis,
and manipulations.
- utility
- : for printing, catalog
handling, and mathematical operations.
- display
- : for plotting, and displaying.
- dish
- : for processing single-dish data.
- atnf
- : contains modules relevant for data from the
Australia Telescope.
- nrao
- : contains modules relevant for data from
NRAO telescopes, currently the GBT and the VLA.
Each package contains a specific set of modules. modules are a group
of closely related applications. For example, the modules of package
Synthesis are:
- calibrater: calibrating UV data
- componentmodels: making source
component models
- imager: imaging and deconvolution, wide-field
imaging, mosaicing, etc..
- simulator: simulating UV and other data
- msplot: plotting visibility data in various ways
Next: Appendix B: Creating your own .aipsrc file
Up: Getting Started in AIPS++
Previous: Frequently Asked Questions
  Contents
Please send questions or comments about AIPS++ to aips2-request@nrao.edu.
Copyright © 1995-2000 Associated Universities Inc.,
Washington, D.C.
Return to AIPS++ Home Page
2006-10-15