Self-calibration pipeline to process VLA data, using CASA tools and WSClean.
- Begins imaging in WSClean using high DR parameters (multi-term, multi-scale, deep clean)
- Uses model to calibrate on chosen solution intervals and modes
- (optional) Performs statistical flagging on RESIDUAL_DATA column
- (optional) Smoothes short-timescale solutions for less noise
-Singularity
-Singularity container from https://tikk3r.github.io/flocs/
-CASA
-Python (version 3 and above)
-
Initiate a CASA environment
module load casa -
Ensure that PYTHONPATH points to the CASA installation python
export PYTHONPATH="/soft/casa-latest/bin/python3" -
Edit vla_selfcal.py so that singularity and CASA paths point to your installations. Place paths to MS and output directories
-
Run
python3 vla_selfcal.py <ms> <output_dir> <config.txt>
Basic example of running the pipeline on JVLA Ku-band C-array data on the bright radio source 3C 123, using 5 cycles with just phase calibration.
