Transients Pipeline

The Transients Pipeline (or "TraP") is a Python based system for detecting and responding to transient and variable sources in a stream of astronomical images. It primarily targets LOFAR data, but is also applicable to a range of other instruments.

Documentation: https://transients-pipeline.readthedocs.io/en/latest/

This is a rework of the original package hosted here: https://github.com/transientskp/tkp An overview of the package and it's initial design can be found in the original TraP paper. If you make use of TraP in work leading to a publication, we ask that you cite this reference.