Features
AIPS++ provides facilities for calibration, editing, image formation, image enhancement, and analysis of images and other astronomical data. A major focus is on reduction of data from both single-dish and aperture synthesis radio telescopes. Although the tools provided in AIPS++ are mainly designed for processing data from varieties of radio telescopes, the package is expected to also be useful for processing other types of astronomical data and images. However, the reduction of most data from imaging array detectors is performed using IRAF instead.
AIPS++ is structured as a library of tools at the lower levels, designed to replace AIPS of more monolithic applications. In general, the counterpart of an AIPS task is an AIPS++ tool function, although the toolkit structure of AIPS++ will generally mean that these functions are more fine-grained, except for the more integrated tools at the higher levels (such as map). The counterparts of AIPS adverbs are the parameters of AIPS++tool functions. The command-line interpreter in AIPS is POPS, while the counterpart in AIPS++ is Glish. The code used as standard in most astronomical institutes is still AIPS, as AIPS++ is usually not yet considered sufficiently reliable and usable.
Like most research astronomy software, it is available for all major operating systems except Microsoft Windows.
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