#Casa software mac os

flagdata: improvements and bug fixes were implemented.importasdm/exportasdm: parameters 'showversion' and 'useversion' have been removed.T+dT timerange selection improved in accuracy.sdintimaging: now adds information to the history of produced images.caltables: storage of frequency meta information improved.imhead: updated to display micro-arcsecond precision.fringefit: memory usage has been reduced, allowing larger datasets to be processed.gencal: a new caltype parameter 'jyperk' has been added.tclean: now handles mixed polarization setups.

plotms: calibration table averaging with channel selection is now supported.plotcal/plotms: funtionality for plotcal has been migrated to plotms, and plotcal was deprecated.

#Casa software mac os

OS Support: RedHat 8 and Mac OS with Python 3.8, for monolithic and modular versions.

The CASA software can process data from both single-dish and aperture-synthesis telescopes, and one of its core functionalities is to support the data reduction and imaging pipelines for ALMA, VLA and the VLA Sky Survey ( VLASS).

Jansky Very Large Array ( VLA), and is frequently used also for other radio telescopes. CASA, the Common Astronomy Software Applications package, is the primary data processing software for the Atacama Large Millimeter/submillimeter Array ( ALMA) and NSF's Karl G.