(C) SARAO, Radio Astronomy Research Group
(C) Benjamin Hugo
The Astronomer, by Vermeer
This is the home of the VermeerKAT pipeline. The goal of this project is two-fold
Currently the pipeline does flagging, transfer calibration, polarization calibration and 3GC self-calibration. The various tasks are available through the vermeerkat
wrapper. Use vermeerkat --help
The Basic Apply Transfer (BAT) pipeline is feature complete. The pipeline uses the RARG tricolour flagger in combination with CASA and WSClean to perform transfer calibration (1GC). BAT can be invoked through:
vermeerkat transfer --help
Fleetingpol is now part of the Vermeerkat suite. You can run this standalone on any bandpass corrected dataset (like that produced from BAT which has transferred the solutions to 3C286 / 3C138), with the caveat that the corrected calibrator data is all stored in CORRECTED_DATA). I recommend that you mark your crosshand phase calibrator as an ALTCAL in BAT to calibrate keep the system phased on the crosshand calibrator. See available options from
vermeerkat poltransfer --help
NOTE: A known issue with MeerKAT data is that both Q and V is flipped in sign with respect to the IEEE convention. After calibration it is necessary to flip signs in analysis. The fleetingpol pipeline forms a SKY_CORRECTED_DATA column which can be used for imaging in the derotated sky frame. Any further self calibration should be performed with the CORRECTED_DATA column. Ideally this pipeline is run post self-calibration of the phase of the target field.
The Introspect self-calibration pipeline is a configurable self-calibration pipeline with capacity to apply delay, phase and amplitude direction dependent self-calibration using CASA, CubiCal and DDFacet. A recipe can be specified as follows:
p(35,256s),p(25,64s),dp(15,16s),ap(7,16s),i(CORRECTED_DATA,0.0),s(CORRECTED_DATA),i(SUBTRACTED_DATA,0.0)
Full help is available by running
vermeerkat selfcal --help
You need to have casacore-data installed on your system. The package should be installed via pip, preferably into a virtual environment
The latest version of github.com/ratt-ru/stimela.git should be installed in the same virtual environment.
Here is full 800 MHz Triangulum Australis from MeerKAT ROACH II 16 antenna data (AR. 1.5):
ROACH II MK16 Triangulum Australis low mass cluster with patch-based (marked in yellow convex hull) dE calibration applied through CubiCal (https://github.com/ratt-ru/CubiCal.git)