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IMAGER is an interferometric imaging package, tailored for usage simplicity and efficiency for multi-spectral data sets.
for new users
IMAGER is build on the GILDAS infrastructure, namely its command line interpreter SIC and its graphics package GREG. Please refer to their respective documentations for details on the Gildas web site (https://www.iram.fr/IRAMFR/GILDAS/).
for previous users of MAPPING
IMAGER is *** NOT *** MAPPING
IMAGER was created because the initial infrastructure for imaging in the MAPPING1program was not adapted to the implementation of imaging methods that became possible and/or were required for NOEMA (and useable for ALMA), such as self-calibration, wide band imaging, or routine processing of Mosaics and Short spacings.
The
IMAGER design takes great care of efficiency, by using parallel
programming and minimizing Input/Output on files. This lead to a
concept with a single
READ of data, a few (in general only 2)
simple processing commands with built-in intelligent parameter guesses,
a visual user control, and a single
WRITE of the results once the
user is satisfied of it.
IMAGER was initially derived from MAPPING by S. Guilloteau, and subsequently extended with many new functionalities.
T. Jacq and E. di Folco made numerous suggestions about the user interface, and helped testing and documenting the program.
Although many basic algorithms from MAPPING were re-used, a large number of improvements (in particular for speed using parallel programming) (and some bug corrections) were performed. New methods were also developped, tested and implemented.
We took the opportunity to revise and streamline the user interface, providing access to all tools through simple commands. A special effort was put on the visualization tools, that provide enhanced speed and capabilities, yet preserving a very high level of compatibility with those previously offered in MAPPING.