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20.1 AIPS
AIPS, NRAO's Astronomical Image Processing System, is a set of
programs for the analysis of continuum and line observations, and is
widely used with VLBA and VLBI data. These programs
are available for a wide range of computer operating systems, including
various flavors of Linux and the Mac-OS/X operating system.
Sections 24.1 and 24.3 give contact
information. Extensive online internal documentation can be accessed
within AIPS. An entire chapter in the AIPS Cookbook (NRAO staff,
2007) provides useful ``how-to'' guidance for those reducing VLBI
data, including discussion of VLBA calibration transfer, space VLBI,
polarimetry, and phase referencing. Appendix C of the AIPS Cookbook
provides a step-by-step guide to calibrating many types of VLBA data
sets in AIPS, employing simple VLBA utilities, including calibration
modifications for VLBA+VLA datasets. A new ``frozen'' version of AIPS
(currently 31DEC08) is produced each year, and a newer version
(currently 31DEC09) is updated and made available throughout the calendar
year. Observers are encouraged to use a very recent version of AIPS,
since only these can properly handle data from the DiFX software
correlator, and new capabilities, such as simplified data-reduction
procedures and improved astrometric calibration, are implemented
frequently.
Next: 20.2 CASA
Up: 20 POST-PROCESSING SOFTWARE
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Stephan Witz
2010-09-21