IRAF is a powerful and comprehensive package for reducing and analysing optical astonomical data. It was developed at the National Optical Astronomy Observatory (NOAO) in Tucson, Arizona and is now in widespread use around the world. Users run IRAF applications from a command line interface called CL. It is also possible to run Figaro from CL. There are (at least) two reasons for wanting to do so:
The Figaro and standard IRAF applications can inter-operate, so a given dataset can be processed using a mixture of Figaro and standard IRAF applications.
Figaro and IRAF intrinsically use different data formats (the Figaro
formats are described in Section
). However, when Figaro
is run from the IRAF CL the system is set up so that the Figaro
applications automatically convert to and from the IRAF format on
input and output respectively. Thus, you will see only data files
in the native IRAF format. This conversion happens automatically
and invisibly and as a user you will not normally need to be
concerned about how it is done. However, one caveat that you should
be aware of is that the native Figaro format is more `capable', in
the sense that it can contain more auxiliary information such as
quality arrays, error arrays, etc. than the IRAF format. Thus, when
datasets are written using the IRAF format some of this auxiliary
information can be lost.
The procedure to run Figaro from within IRAF is as follows.
cl> figaro
(here `cl>' is the CL prompt, not something that you type
in). A welcome message and list of commands will be displayed and
the Figaro applications can simply be run.
There are various points which it is useful to be aware of when running Figaro, or other Starlink applications, from within CL. The details are discussed in SUN/217.
FIGARO A general data reduction system