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Before any data can be processed by AIPS, they must first be imported into the system's own data areas, usually in [[FITS]] format. The FITS standard was agreed in 1979 and its development is inseparable from that of AIPS. The data can henceforth be processed using a large number (>530) of individual programs, each of which performs a specific task e.g. producing an image from a calibrated data set. Together these allow a user to visualize, edit and calibrate a data set and subsequently make images or fit models. A number of analysis tasks are included (e.g. Gaussian fitting to images or spectra) as well as the possibility to make publication-quality plots.
Extensive help is available to AIPS users, with detailed information on each parameter and task viewable from the command line. There is also a [[user guide]], the AIPS Cookbook, which is built around examples (recipes) of how to run the various tasks. It is available on-line, as well as being packaged with AIPS in
==Primatology==
Although briefly known as RANCID<ref>{{cite journal|last1=Greisen|first1=Eric|editor1-last=Heck|editor1-first=André|title=AIPS, the VLA, and the VLBA|journal=Information Handling in Astronomy - Historical Vistas|date=2003|page=285|publisher=Kluwer}}</ref>, the eventual choice of name has led to a preponderance of primate-based humour in and around AIPS. The Cookbook contains "additional recipes",
==References==
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