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The pipeline has been ported to work with CASA 5+ versions, and works with latest version available v5.4
It can calibrate spectral line data.
It can calibrate all frequency bands: C, L and K band.
Accepts pseudo wideband processing (C-band data from 4.5 to 7.5 GHz).
Pipeline can search for observatory logs of slewing antennas and flag off-source visibilities.
Multiprocessing CASA (mpicasa) working properly.
The weblog includes a summary page with real-time information of steps executed, main parameters and access to all processing and calibration parameters used.
Add-on script under development to self-calibrate sources processed with the pipeline.
Implemented automatic Lovell dropout scans detection and flagging.
The pipeline accepts models of the structure of the phase calibrators.
Added possibility to use any flux calibrator and to set the flux manually.
New autoflagging procedures (TFCROP, and optionally RFLAG) during calibration.
Use phase solution tables to flag calibrator visibilities.
More complete plots of calibration tables.
Pipeline can correct phase centre of sources, or generate new phase centres for other sources in the FoV.