This page provides a compliation of several uGMRT data-reduction pipelines for continuum data, both total intensity and polarization, as well spectral line data. These pipelines have been developed by individual astronomers at NCRA-TIFR, India. If you make use of these pipelines, please cite the references mentioned along with the links.
https://github.com/ruta-k/uGMRT-pipeline
The pipeline is described in detail in the following paper:
https://ui.adsabs.harvard.edu/abs/2020arXiv201000196K/abstract
https://drive.google.com/file/d/1_s0_PwRuESHfrORN-Rok3VXIytOTYAU5/view
This pipeline has so far been tested extensively on Band 4 uGMRT data. Steps for running this pipeline are here:
https://drive.google.com/file/d/1afkoHsAde-mM3bJnKPYS9fqsbJZcEH4l/view
The pipeline is described in detail in the following paper. If you use this pipeline for publication purpose, kindly cite this paper:
https://ui.adsabs.harvard.edu/abs/2021MNRAS.507..991S/abstract
Polarization modelling for 3C286, 3C48, and 3C138 included within the pipeline. This pipeline has so far been tested extensively on Band 4 uGMRT data. Please cite the following paper if you use this pipeline for publication purposes.
This pipeline is suitable for point source dominated fields. For imaging extended emission, CAPTURE is recommended which has smart flagging options for retaining extended emission.
http://www.ncra.tifr.res.in/~ishwar/pipeline.html
This pipeline uses AIPS to carry out all the calibration and few rounds of imaging and self-calibration, after which the final imaging is carried out in CASA using the MT-MFS algorithm. CASA automatic flagging algorithms, namely 'tfcrop' and 'rflag' are also made use of. When making use of this pipeline, please cite Biny Sebastian's PhD thesis.
https://github.com/binysebastian/aipsscriptwriter
This pipeline is targeted towards HI spectral line imaging.