Image may be NSFW.
Clik here to view.© Cristiana Spingola
The image is of a gravitational lens with emission from four images of the lensed source (A through D) and from the lensing galaxy. The data were obtained with the VLBA at L-band, in a 12 hour run. The data was amplitude calibrated, phase calibrated with the new fringe fitter, imaged and cleaned fully in CASA.
The new CASA VLBI tools consist of a newly implemented fringe fitting task, upgrades of existing tasks to handle VLBI data, and a collection of scripts to ensure proper handling and import of the meta-data. The new fringefit task is based on the AIPS FRING task. The development of the CASA VLBI tools was started for the ERC BlackHoleCam project, with financial support from SKA-NL. It currently continues under the RadioNet RINGS JRA, with help from the CASA developers at NRAO, Socorro.
Further testing and development is still ongoing, e.g. prototyping a dispersive delay fit has started, and a next step will be the handling of discontinuous frequency bands. The current plan is to provide a beta-version of the VLBI tools in CASA 5.3.