SKA SDP Spectral Line Imaging Pipeline

The Spectral Line Imaging pipeline has following steps (in its default order):

1. Read visibilities from MSv4 formatted zarr file (also called "processing set" in xradio terms)

2. Predict model visibilities from continuum images

3. Perform continuum subtraction on visibilities using model visibilities

4. (Optional) Perform flagging of visibilities

5. Run imaging to generate spectral FITS cubes as output.

Readme

• Getting Started
• Developer Guide

Releases

• Changelog

Contents

• Running on a Local Dask Cluster
• Benchmarking Pipeline
• Stages and configurations

API

• API