CIMG
The Continuum Imaging Pipeline (CIMG) produces contimuum images from the pre-processed target field visibilities (generated by BPP) and the gain table and facet regions generated by the self-calibration pipeline (ICAL) using WSClean.
Current outputs include model images, residual images and restored images. Work is planned to support stacking images into a cube.
CIMG runs either on a single or multiple nodes (using MPI) and selected WSClean parameters are configured using a YAML file as input. It can optionally accept a mask. CIMG is written in Python and orchestrated with prefect. Its progress can be monitored using the prefect UI.
flowchart LR
input_ms@{ shape: disk, label: "Pre-processed <br> Visibilities <br> (Target)"}
solutions@{ shape: disk, label: "Gain Table (DDE)"}
facet_regions@{ shape: disk, label: "Facet Regions"}
config@{ shape: doc, label: "Configuration"}
ical(("Self-Calibration<br>(ICAL)")) --> solutions & facet_regions
bpp(("Batch Pre-Processing<br>(BPP)")) --> input_ms
subgraph cimg["Continuum Imaging (CIMG)"]
configure@{ shape: rect, label: "Configure pipeline" }
image@{ shape: rect, label: "Run WSClean"}
stack@{ shape: rect, label: "Stack images" }
end
image_cube@{ shape: disk, label: "Image cube"}
images@{ shape: disk, label: "Images"}
config --> configure --> image
input_ms & solutions & facet_regions --> image
image --> images
image -.-> stack -.-> image_cube
style stack fill:stroke-width:2px,stroke-dasharray: 5 5
style image_cube fill:stroke-width:2px,stroke-dasharray: 5 5
Useful Links
Complete the following with relevant links for your pipeline.
Repository: https://gitlab.com/ska-telescope/sdp/science-pipeline-workflows/ska-sdp-cimg
Documentation: https://developer.skao.int/projects/ska-sdp-cimg/en/latest/
Description: Produces continuum images of the sky following self-calibration.
Quickstart: https://developer.skao.int/projects/ska-sdp-cimg/en/latest/quickstart.html
Status: In development
Contact: Team GECKO
Where to get help: #gecko-cimg