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TraP: The LOFAR Transients Pipeline
The LOFAR Transients Pipeline (or "TraP") is a Python and SQL based system for detecting and responding to transient and variable sources in a stream of astronomical images.
- Image processing
- radio astronomy
- Source association
- + 3
- Mako
- PLpgSQL
- Python
- + 1
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eAstroViz
This tool can convert and visualize radio astronomy measurement sets, as well as most LOFAR intermediate data products. It also performs RFI mitigation.
- LOFAR
- radio astronomy
- RFI
- C
- C++
- Cuda
- + 3
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